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You searched for subject:(Accretion Disk). Showing records 1 – 30 of 43 total matches.

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Addis Ababa University

1. HAFTAMU, G/MARIAM. THE CONTRIBUTION OF RADIATION PRESSURE TO THE STABILITY OF A STANDARD THIN KEPLERIAN ACCRETION DISK AROUND A NEUTRON STAR WITH AXISYMMETRIC MAGNETIC FIELD DIPOLE .

Degree: 2012, Addis Ababa University

 In this thesis, we have studied the dynamic properties of an accretion disk formed from the in ow of plasma from a blotted out companion… (more)

Subjects/Keywords: AXISYMMETRIC; KEPLERIAN ACCRETION DISK

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APA · Chicago · MLA · Vancouver · CSE | Export to Zotero / EndNote / Reference Manager

APA (6th Edition):

HAFTAMU, G. (2012). THE CONTRIBUTION OF RADIATION PRESSURE TO THE STABILITY OF A STANDARD THIN KEPLERIAN ACCRETION DISK AROUND A NEUTRON STAR WITH AXISYMMETRIC MAGNETIC FIELD DIPOLE . (Thesis). Addis Ababa University. Retrieved from http://etd.aau.edu.et/dspace/handle/123456789/1280

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Chicago Manual of Style (16th Edition):

HAFTAMU, G/MARIAM. “THE CONTRIBUTION OF RADIATION PRESSURE TO THE STABILITY OF A STANDARD THIN KEPLERIAN ACCRETION DISK AROUND A NEUTRON STAR WITH AXISYMMETRIC MAGNETIC FIELD DIPOLE .” 2012. Thesis, Addis Ababa University. Accessed January 17, 2021. http://etd.aau.edu.et/dspace/handle/123456789/1280.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

MLA Handbook (7th Edition):

HAFTAMU, G/MARIAM. “THE CONTRIBUTION OF RADIATION PRESSURE TO THE STABILITY OF A STANDARD THIN KEPLERIAN ACCRETION DISK AROUND A NEUTRON STAR WITH AXISYMMETRIC MAGNETIC FIELD DIPOLE .” 2012. Web. 17 Jan 2021.

Vancouver:

HAFTAMU G. THE CONTRIBUTION OF RADIATION PRESSURE TO THE STABILITY OF A STANDARD THIN KEPLERIAN ACCRETION DISK AROUND A NEUTRON STAR WITH AXISYMMETRIC MAGNETIC FIELD DIPOLE . [Internet] [Thesis]. Addis Ababa University; 2012. [cited 2021 Jan 17]. Available from: http://etd.aau.edu.et/dspace/handle/123456789/1280.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Council of Science Editors:

HAFTAMU G. THE CONTRIBUTION OF RADIATION PRESSURE TO THE STABILITY OF A STANDARD THIN KEPLERIAN ACCRETION DISK AROUND A NEUTRON STAR WITH AXISYMMETRIC MAGNETIC FIELD DIPOLE . [Thesis]. Addis Ababa University; 2012. Available from: http://etd.aau.edu.et/dspace/handle/123456789/1280

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation


Indian Institute of Science

2. Rajesh, S R. Stability of Accretion Flows And Radiative-Hydrodynamics Around Rotating Black Holes.

Degree: PhD, Faculty of Science, 2013, Indian Institute of Science

 In the case of cold accretion disk, coupling between charge neutral gas and magnetic field is too weak such that the magneto-rotational instability will be… (more)

Subjects/Keywords: Black Holes; Radiative-hydrodynamics; Accretion Flows; Accretion (Astrophysics); Accretion Disc; Accretion Disk - Hydrodynamic Instability; Blackholes; Astrophysics

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APA (6th Edition):

Rajesh, S. R. (2013). Stability of Accretion Flows And Radiative-Hydrodynamics Around Rotating Black Holes. (Doctoral Dissertation). Indian Institute of Science. Retrieved from http://etd.iisc.ac.in/handle/2005/2076

Chicago Manual of Style (16th Edition):

Rajesh, S R. “Stability of Accretion Flows And Radiative-Hydrodynamics Around Rotating Black Holes.” 2013. Doctoral Dissertation, Indian Institute of Science. Accessed January 17, 2021. http://etd.iisc.ac.in/handle/2005/2076.

MLA Handbook (7th Edition):

Rajesh, S R. “Stability of Accretion Flows And Radiative-Hydrodynamics Around Rotating Black Holes.” 2013. Web. 17 Jan 2021.

Vancouver:

Rajesh SR. Stability of Accretion Flows And Radiative-Hydrodynamics Around Rotating Black Holes. [Internet] [Doctoral dissertation]. Indian Institute of Science; 2013. [cited 2021 Jan 17]. Available from: http://etd.iisc.ac.in/handle/2005/2076.

Council of Science Editors:

Rajesh SR. Stability of Accretion Flows And Radiative-Hydrodynamics Around Rotating Black Holes. [Doctoral Dissertation]. Indian Institute of Science; 2013. Available from: http://etd.iisc.ac.in/handle/2005/2076


Addis Ababa University

3. GEREZIHER, HAGOS. THE CONTRIBUTION OF COULOMBIC PRESSURE TO THE STABILITY OF THIN KEPLERIAN ACCRETION DISCS AROUND A NEUTRON STAR WITH AXISYMMETRIC MAGNETIC DIPOLE .

Degree: 2012, Addis Ababa University

 We determine the stability of an axisymmetric geometrically thin and optically thick accretion disc around a magnetized neutron star in the region where gas pressure… (more)

Subjects/Keywords: accretion disc; magnetized neutron star

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APA (6th Edition):

GEREZIHER, H. (2012). THE CONTRIBUTION OF COULOMBIC PRESSURE TO THE STABILITY OF THIN KEPLERIAN ACCRETION DISCS AROUND A NEUTRON STAR WITH AXISYMMETRIC MAGNETIC DIPOLE . (Thesis). Addis Ababa University. Retrieved from http://etd.aau.edu.et/dspace/handle/123456789/1275

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Chicago Manual of Style (16th Edition):

GEREZIHER, HAGOS. “THE CONTRIBUTION OF COULOMBIC PRESSURE TO THE STABILITY OF THIN KEPLERIAN ACCRETION DISCS AROUND A NEUTRON STAR WITH AXISYMMETRIC MAGNETIC DIPOLE .” 2012. Thesis, Addis Ababa University. Accessed January 17, 2021. http://etd.aau.edu.et/dspace/handle/123456789/1275.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

MLA Handbook (7th Edition):

GEREZIHER, HAGOS. “THE CONTRIBUTION OF COULOMBIC PRESSURE TO THE STABILITY OF THIN KEPLERIAN ACCRETION DISCS AROUND A NEUTRON STAR WITH AXISYMMETRIC MAGNETIC DIPOLE .” 2012. Web. 17 Jan 2021.

Vancouver:

GEREZIHER H. THE CONTRIBUTION OF COULOMBIC PRESSURE TO THE STABILITY OF THIN KEPLERIAN ACCRETION DISCS AROUND A NEUTRON STAR WITH AXISYMMETRIC MAGNETIC DIPOLE . [Internet] [Thesis]. Addis Ababa University; 2012. [cited 2021 Jan 17]. Available from: http://etd.aau.edu.et/dspace/handle/123456789/1275.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Council of Science Editors:

GEREZIHER H. THE CONTRIBUTION OF COULOMBIC PRESSURE TO THE STABILITY OF THIN KEPLERIAN ACCRETION DISCS AROUND A NEUTRON STAR WITH AXISYMMETRIC MAGNETIC DIPOLE . [Thesis]. Addis Ababa University; 2012. Available from: http://etd.aau.edu.et/dspace/handle/123456789/1275

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation


Penn State University

4. Flohic, Helene Marie. INTERPRETING DOUBLE-PEAKED EMISSION LINE PROFILE VARIABILITY IN AGNS USING MODELS FOR ACCRETION DISK STRUCTURES .

Degree: 2008, Penn State University

 A subset of Active Galactic Nuclei (AGNs) have broad, double-peaked Balmer emission lines, regarded as the best kinematic evidence for the production of broad lines… (more)

Subjects/Keywords: AGNs; accretion disk

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APA (6th Edition):

Flohic, H. M. (2008). INTERPRETING DOUBLE-PEAKED EMISSION LINE PROFILE VARIABILITY IN AGNS USING MODELS FOR ACCRETION DISK STRUCTURES . (Thesis). Penn State University. Retrieved from https://submit-etda.libraries.psu.edu/catalog/9233

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Chicago Manual of Style (16th Edition):

Flohic, Helene Marie. “INTERPRETING DOUBLE-PEAKED EMISSION LINE PROFILE VARIABILITY IN AGNS USING MODELS FOR ACCRETION DISK STRUCTURES .” 2008. Thesis, Penn State University. Accessed January 17, 2021. https://submit-etda.libraries.psu.edu/catalog/9233.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

MLA Handbook (7th Edition):

Flohic, Helene Marie. “INTERPRETING DOUBLE-PEAKED EMISSION LINE PROFILE VARIABILITY IN AGNS USING MODELS FOR ACCRETION DISK STRUCTURES .” 2008. Web. 17 Jan 2021.

Vancouver:

Flohic HM. INTERPRETING DOUBLE-PEAKED EMISSION LINE PROFILE VARIABILITY IN AGNS USING MODELS FOR ACCRETION DISK STRUCTURES . [Internet] [Thesis]. Penn State University; 2008. [cited 2021 Jan 17]. Available from: https://submit-etda.libraries.psu.edu/catalog/9233.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Council of Science Editors:

Flohic HM. INTERPRETING DOUBLE-PEAKED EMISSION LINE PROFILE VARIABILITY IN AGNS USING MODELS FOR ACCRETION DISK STRUCTURES . [Thesis]. Penn State University; 2008. Available from: https://submit-etda.libraries.psu.edu/catalog/9233

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation


University of Guelph

5. Russell, John L. Development of a Self-Consistent Gas Accretion Model for Simulating Gas Giant Formation in Protoplanetary Disks.

Degree: MS, Department of Physics, 2011, University of Guelph

 The number of extrasolar planet discoveries has increased dramatically over the last 15 years. Nearly 700 exoplanets have currently been observed through a variety of… (more)

Subjects/Keywords: astrophysics; accretion disk; protoplanetary disk; planet formation; gas giant; exoplanet; accretion; planets; FARGO

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APA (6th Edition):

Russell, J. L. (2011). Development of a Self-Consistent Gas Accretion Model for Simulating Gas Giant Formation in Protoplanetary Disks. (Masters Thesis). University of Guelph. Retrieved from https://atrium.lib.uoguelph.ca/xmlui/handle/10214/3212

Chicago Manual of Style (16th Edition):

Russell, John L. “Development of a Self-Consistent Gas Accretion Model for Simulating Gas Giant Formation in Protoplanetary Disks.” 2011. Masters Thesis, University of Guelph. Accessed January 17, 2021. https://atrium.lib.uoguelph.ca/xmlui/handle/10214/3212.

MLA Handbook (7th Edition):

Russell, John L. “Development of a Self-Consistent Gas Accretion Model for Simulating Gas Giant Formation in Protoplanetary Disks.” 2011. Web. 17 Jan 2021.

Vancouver:

Russell JL. Development of a Self-Consistent Gas Accretion Model for Simulating Gas Giant Formation in Protoplanetary Disks. [Internet] [Masters thesis]. University of Guelph; 2011. [cited 2021 Jan 17]. Available from: https://atrium.lib.uoguelph.ca/xmlui/handle/10214/3212.

Council of Science Editors:

Russell JL. Development of a Self-Consistent Gas Accretion Model for Simulating Gas Giant Formation in Protoplanetary Disks. [Masters Thesis]. University of Guelph; 2011. Available from: https://atrium.lib.uoguelph.ca/xmlui/handle/10214/3212


University of Cambridge

6. Kosec, Peter. Studying accretion disc winds with X-ray spectroscopy.

Degree: PhD, 2020, University of Cambridge

 In this thesis I present the results of my PhD research into the physics of accretion (infall) and ejection (outflow) of matter in compact objects.… (more)

Subjects/Keywords: X-ray Astronomy; Accretion; Neutron Stars; Black Holes; Accretion Disc Winds

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APA (6th Edition):

Kosec, P. (2020). Studying accretion disc winds with X-ray spectroscopy. (Doctoral Dissertation). University of Cambridge. Retrieved from https://doi.org/10.17863/CAM.57704 ; https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.814569

Chicago Manual of Style (16th Edition):

Kosec, Peter. “Studying accretion disc winds with X-ray spectroscopy.” 2020. Doctoral Dissertation, University of Cambridge. Accessed January 17, 2021. https://doi.org/10.17863/CAM.57704 ; https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.814569.

MLA Handbook (7th Edition):

Kosec, Peter. “Studying accretion disc winds with X-ray spectroscopy.” 2020. Web. 17 Jan 2021.

Vancouver:

Kosec P. Studying accretion disc winds with X-ray spectroscopy. [Internet] [Doctoral dissertation]. University of Cambridge; 2020. [cited 2021 Jan 17]. Available from: https://doi.org/10.17863/CAM.57704 ; https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.814569.

Council of Science Editors:

Kosec P. Studying accretion disc winds with X-ray spectroscopy. [Doctoral Dissertation]. University of Cambridge; 2020. Available from: https://doi.org/10.17863/CAM.57704 ; https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.814569


University of Cambridge

7. Kosec, Peter. Studying Accretion Disc Winds with X-ray Spectroscopy.

Degree: PhD, 2020, University of Cambridge

 In this thesis I present the results of my PhD research into the physics of accretion (infall) and ejection (outflow) of matter in compact objects.… (more)

Subjects/Keywords: X-ray Astronomy; Accretion; Neutron Stars; Black Holes; Accretion Disc Winds

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APA · Chicago · MLA · Vancouver · CSE | Export to Zotero / EndNote / Reference Manager

APA (6th Edition):

Kosec, P. (2020). Studying Accretion Disc Winds with X-ray Spectroscopy. (Doctoral Dissertation). University of Cambridge. Retrieved from https://www.repository.cam.ac.uk/handle/1810/310607

Chicago Manual of Style (16th Edition):

Kosec, Peter. “Studying Accretion Disc Winds with X-ray Spectroscopy.” 2020. Doctoral Dissertation, University of Cambridge. Accessed January 17, 2021. https://www.repository.cam.ac.uk/handle/1810/310607.

MLA Handbook (7th Edition):

Kosec, Peter. “Studying Accretion Disc Winds with X-ray Spectroscopy.” 2020. Web. 17 Jan 2021.

Vancouver:

Kosec P. Studying Accretion Disc Winds with X-ray Spectroscopy. [Internet] [Doctoral dissertation]. University of Cambridge; 2020. [cited 2021 Jan 17]. Available from: https://www.repository.cam.ac.uk/handle/1810/310607.

Council of Science Editors:

Kosec P. Studying Accretion Disc Winds with X-ray Spectroscopy. [Doctoral Dissertation]. University of Cambridge; 2020. Available from: https://www.repository.cam.ac.uk/handle/1810/310607

8. Kadowaki, Luis Henrique Sinki. Reconexão magnética em discos de acreção e seus efeitos sobre a formação e aceleração de jatos: um estudo teórico-numérico.

Degree: Mestrado, Astronomia, 2011, University of São Paulo

 Jatos e discos de acreção associados a objetos galácticos e extragalácticos tais como, microquasares (i.e., buracos negros de massa estelar presentes em alguns sistemas binários… (more)

Subjects/Keywords: Accretion disk; Campos Magnéticos; Discos de acreção; Magnetic fields; Magnetohidrodinâmica; Magnetohydrodynamics

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APA (6th Edition):

Kadowaki, L. H. S. (2011). Reconexão magnética em discos de acreção e seus efeitos sobre a formação e aceleração de jatos: um estudo teórico-numérico. (Masters Thesis). University of São Paulo. Retrieved from http://www.teses.usp.br/teses/disponiveis/14/14131/tde-15012012-121521/ ;

Chicago Manual of Style (16th Edition):

Kadowaki, Luis Henrique Sinki. “Reconexão magnética em discos de acreção e seus efeitos sobre a formação e aceleração de jatos: um estudo teórico-numérico.” 2011. Masters Thesis, University of São Paulo. Accessed January 17, 2021. http://www.teses.usp.br/teses/disponiveis/14/14131/tde-15012012-121521/ ;.

MLA Handbook (7th Edition):

Kadowaki, Luis Henrique Sinki. “Reconexão magnética em discos de acreção e seus efeitos sobre a formação e aceleração de jatos: um estudo teórico-numérico.” 2011. Web. 17 Jan 2021.

Vancouver:

Kadowaki LHS. Reconexão magnética em discos de acreção e seus efeitos sobre a formação e aceleração de jatos: um estudo teórico-numérico. [Internet] [Masters thesis]. University of São Paulo; 2011. [cited 2021 Jan 17]. Available from: http://www.teses.usp.br/teses/disponiveis/14/14131/tde-15012012-121521/ ;.

Council of Science Editors:

Kadowaki LHS. Reconexão magnética em discos de acreção e seus efeitos sobre a formação e aceleração de jatos: um estudo teórico-numérico. [Masters Thesis]. University of São Paulo; 2011. Available from: http://www.teses.usp.br/teses/disponiveis/14/14131/tde-15012012-121521/ ;


McMaster University

9. Jackel, Benjamin. Magnetic Dynamos: How Do They Even Work?.

Degree: PhD, 2015, McMaster University

The origin of cosmic magnetic fields is a important area of astrophysics. The process by which they are created falls under the heading of dynamo… (more)

Subjects/Keywords: Accretion Disk; Magnetic Dynamo; magnetohydrodynamics; Mean Field Theory

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APA (6th Edition):

Jackel, B. (2015). Magnetic Dynamos: How Do They Even Work?. (Doctoral Dissertation). McMaster University. Retrieved from http://hdl.handle.net/11375/18299

Chicago Manual of Style (16th Edition):

Jackel, Benjamin. “Magnetic Dynamos: How Do They Even Work?.” 2015. Doctoral Dissertation, McMaster University. Accessed January 17, 2021. http://hdl.handle.net/11375/18299.

MLA Handbook (7th Edition):

Jackel, Benjamin. “Magnetic Dynamos: How Do They Even Work?.” 2015. Web. 17 Jan 2021.

Vancouver:

Jackel B. Magnetic Dynamos: How Do They Even Work?. [Internet] [Doctoral dissertation]. McMaster University; 2015. [cited 2021 Jan 17]. Available from: http://hdl.handle.net/11375/18299.

Council of Science Editors:

Jackel B. Magnetic Dynamos: How Do They Even Work?. [Doctoral Dissertation]. McMaster University; 2015. Available from: http://hdl.handle.net/11375/18299


Texas Tech University

10. Osler, Arlo Ray. The Lack of Radio Jet Emissions from 4U 1957+11: New Constraints on Jet Production from Thin Accretion Disks.

Degree: MS, Physics, 2017, Texas Tech University

 Radio emission from the jets of soft state stellar mass black hole X-ray binaries is believed to be suppressed by more than a factor of… (more)

Subjects/Keywords: Soft state; Accretion disk; Radio jet emission; 4U 1957+11

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APA (6th Edition):

Osler, A. R. (2017). The Lack of Radio Jet Emissions from 4U 1957+11: New Constraints on Jet Production from Thin Accretion Disks. (Masters Thesis). Texas Tech University. Retrieved from http://hdl.handle.net/2346/82047

Chicago Manual of Style (16th Edition):

Osler, Arlo Ray. “The Lack of Radio Jet Emissions from 4U 1957+11: New Constraints on Jet Production from Thin Accretion Disks.” 2017. Masters Thesis, Texas Tech University. Accessed January 17, 2021. http://hdl.handle.net/2346/82047.

MLA Handbook (7th Edition):

Osler, Arlo Ray. “The Lack of Radio Jet Emissions from 4U 1957+11: New Constraints on Jet Production from Thin Accretion Disks.” 2017. Web. 17 Jan 2021.

Vancouver:

Osler AR. The Lack of Radio Jet Emissions from 4U 1957+11: New Constraints on Jet Production from Thin Accretion Disks. [Internet] [Masters thesis]. Texas Tech University; 2017. [cited 2021 Jan 17]. Available from: http://hdl.handle.net/2346/82047.

Council of Science Editors:

Osler AR. The Lack of Radio Jet Emissions from 4U 1957+11: New Constraints on Jet Production from Thin Accretion Disks. [Masters Thesis]. Texas Tech University; 2017. Available from: http://hdl.handle.net/2346/82047


University of the Western Cape

11. Kolwa, Sthabile. The effects of environment on radio-loud AGN activity in Stripe 82 .

Degree: 2016, University of the Western Cape

 We investigate the link between environment and radiative accretion efficiency using a sample of 8946 radio-loud AGN detected at 1 − 2 GHz in the… (more)

Subjects/Keywords: Photometry - infrared; Accretion-disk physics; Galaxies; Galaxies – Evolution

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APA (6th Edition):

Kolwa, S. (2016). The effects of environment on radio-loud AGN activity in Stripe 82 . (Thesis). University of the Western Cape. Retrieved from http://hdl.handle.net/11394/5318

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Chicago Manual of Style (16th Edition):

Kolwa, Sthabile. “The effects of environment on radio-loud AGN activity in Stripe 82 .” 2016. Thesis, University of the Western Cape. Accessed January 17, 2021. http://hdl.handle.net/11394/5318.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

MLA Handbook (7th Edition):

Kolwa, Sthabile. “The effects of environment on radio-loud AGN activity in Stripe 82 .” 2016. Web. 17 Jan 2021.

Vancouver:

Kolwa S. The effects of environment on radio-loud AGN activity in Stripe 82 . [Internet] [Thesis]. University of the Western Cape; 2016. [cited 2021 Jan 17]. Available from: http://hdl.handle.net/11394/5318.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Council of Science Editors:

Kolwa S. The effects of environment on radio-loud AGN activity in Stripe 82 . [Thesis]. University of the Western Cape; 2016. Available from: http://hdl.handle.net/11394/5318

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation


University of Rochester

12. Li, Shule. Heterogeneous flow in interstellar medium and star formation.

Degree: PhD, 2014, University of Rochester

 Almost all interstellar objects contain inherent inhomogeneity. The inhomogeneity can manifest in many different ways, such as the uneven matter distribution in a molecular cloud,… (more)

Subjects/Keywords: Accretion disc; Heterogeneous flow; Interstellar medium; Magneto-hydrodynamics; Shock; Star formation

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APA (6th Edition):

Li, S. (2014). Heterogeneous flow in interstellar medium and star formation. (Doctoral Dissertation). University of Rochester. Retrieved from http://hdl.handle.net/1802/28862

Chicago Manual of Style (16th Edition):

Li, Shule. “Heterogeneous flow in interstellar medium and star formation.” 2014. Doctoral Dissertation, University of Rochester. Accessed January 17, 2021. http://hdl.handle.net/1802/28862.

MLA Handbook (7th Edition):

Li, Shule. “Heterogeneous flow in interstellar medium and star formation.” 2014. Web. 17 Jan 2021.

Vancouver:

Li S. Heterogeneous flow in interstellar medium and star formation. [Internet] [Doctoral dissertation]. University of Rochester; 2014. [cited 2021 Jan 17]. Available from: http://hdl.handle.net/1802/28862.

Council of Science Editors:

Li S. Heterogeneous flow in interstellar medium and star formation. [Doctoral Dissertation]. University of Rochester; 2014. Available from: http://hdl.handle.net/1802/28862


University of Rochester

13. Pecaut, Mark (1975 - ). The star-formation history and accretion disk fraction of the Scorpius-Centaurus OB Association.

Degree: PhD, 2013, University of Rochester

 We present a study of the star-formation history and accretion disk fraction of ∼0.6- 1.8 M⊙ stars in the nearest OB Association, Scorpius-Centaurus (Sco-Cen; 10-20… (more)

Subjects/Keywords: Accretion disk fraction; Intrinsic colors; Pre-main sequence stars; Scorpius-Centaurus; Stellar ages; Stellar temperatures

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APA (6th Edition):

Pecaut, M. (. -. ). (2013). The star-formation history and accretion disk fraction of the Scorpius-Centaurus OB Association. (Doctoral Dissertation). University of Rochester. Retrieved from http://hdl.handle.net/1802/27871

Chicago Manual of Style (16th Edition):

Pecaut, Mark (1975 - ). “The star-formation history and accretion disk fraction of the Scorpius-Centaurus OB Association.” 2013. Doctoral Dissertation, University of Rochester. Accessed January 17, 2021. http://hdl.handle.net/1802/27871.

MLA Handbook (7th Edition):

Pecaut, Mark (1975 - ). “The star-formation history and accretion disk fraction of the Scorpius-Centaurus OB Association.” 2013. Web. 17 Jan 2021.

Vancouver:

Pecaut M(-). The star-formation history and accretion disk fraction of the Scorpius-Centaurus OB Association. [Internet] [Doctoral dissertation]. University of Rochester; 2013. [cited 2021 Jan 17]. Available from: http://hdl.handle.net/1802/27871.

Council of Science Editors:

Pecaut M(-). The star-formation history and accretion disk fraction of the Scorpius-Centaurus OB Association. [Doctoral Dissertation]. University of Rochester; 2013. Available from: http://hdl.handle.net/1802/27871


University of Michigan

14. Zhu, Zhaohuan. Confronting FU Orionis Outbursts and Pre/transitional Disks: Protostellar/ protoplanetary Disk Structure and Evolution.

Degree: PhD, Astronomy and Astrophysics, 2011, University of Michigan

 The mechanisms and efficiencies of mass transport in accretion disks can be best constrained by studying their time-dependent behavior. For the first part of my… (more)

Subjects/Keywords: Star Formation; Planet Formation; Episodic Accretion; Outburst; Magnetorotational Instability; Planet Disk Interaction; Astronomy; Science

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APA (6th Edition):

Zhu, Z. (2011). Confronting FU Orionis Outbursts and Pre/transitional Disks: Protostellar/ protoplanetary Disk Structure and Evolution. (Doctoral Dissertation). University of Michigan. Retrieved from http://hdl.handle.net/2027.42/86332

Chicago Manual of Style (16th Edition):

Zhu, Zhaohuan. “Confronting FU Orionis Outbursts and Pre/transitional Disks: Protostellar/ protoplanetary Disk Structure and Evolution.” 2011. Doctoral Dissertation, University of Michigan. Accessed January 17, 2021. http://hdl.handle.net/2027.42/86332.

MLA Handbook (7th Edition):

Zhu, Zhaohuan. “Confronting FU Orionis Outbursts and Pre/transitional Disks: Protostellar/ protoplanetary Disk Structure and Evolution.” 2011. Web. 17 Jan 2021.

Vancouver:

Zhu Z. Confronting FU Orionis Outbursts and Pre/transitional Disks: Protostellar/ protoplanetary Disk Structure and Evolution. [Internet] [Doctoral dissertation]. University of Michigan; 2011. [cited 2021 Jan 17]. Available from: http://hdl.handle.net/2027.42/86332.

Council of Science Editors:

Zhu Z. Confronting FU Orionis Outbursts and Pre/transitional Disks: Protostellar/ protoplanetary Disk Structure and Evolution. [Doctoral Dissertation]. University of Michigan; 2011. Available from: http://hdl.handle.net/2027.42/86332


Université de Bordeaux I

15. Trova, Audrey. Gravité des systèmes verticalement homogènes : applications aux disques astrophysiques : Gravity of vertically homogeneous systems : application to astrophysical disks.

Degree: Docteur es, Astrophysique, 2013, Université de Bordeaux I

 La gravitation joue un rôle important dans de nombreux domaines de l'astrophysique : elle assure notamment la cohésion et la stabilité des planètes, des étoiles… (more)

Subjects/Keywords: Gravitation; Disque d'accretion; Methode analytique; Methode numérique; Gravitation; Accretion disk; Analytical method; Numerical method

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APA (6th Edition):

Trova, A. (2013). Gravité des systèmes verticalement homogènes : applications aux disques astrophysiques : Gravity of vertically homogeneous systems : application to astrophysical disks. (Doctoral Dissertation). Université de Bordeaux I. Retrieved from http://www.theses.fr/2013BOR14902

Chicago Manual of Style (16th Edition):

Trova, Audrey. “Gravité des systèmes verticalement homogènes : applications aux disques astrophysiques : Gravity of vertically homogeneous systems : application to astrophysical disks.” 2013. Doctoral Dissertation, Université de Bordeaux I. Accessed January 17, 2021. http://www.theses.fr/2013BOR14902.

MLA Handbook (7th Edition):

Trova, Audrey. “Gravité des systèmes verticalement homogènes : applications aux disques astrophysiques : Gravity of vertically homogeneous systems : application to astrophysical disks.” 2013. Web. 17 Jan 2021.

Vancouver:

Trova A. Gravité des systèmes verticalement homogènes : applications aux disques astrophysiques : Gravity of vertically homogeneous systems : application to astrophysical disks. [Internet] [Doctoral dissertation]. Université de Bordeaux I; 2013. [cited 2021 Jan 17]. Available from: http://www.theses.fr/2013BOR14902.

Council of Science Editors:

Trova A. Gravité des systèmes verticalement homogènes : applications aux disques astrophysiques : Gravity of vertically homogeneous systems : application to astrophysical disks. [Doctoral Dissertation]. Université de Bordeaux I; 2013. Available from: http://www.theses.fr/2013BOR14902

16. Belyaev, Mikhail. Dynamics of Thin Astrophysical Boundary Layers .

Degree: PhD, 2013, Princeton University

 We study the modal structure and angular momentum transport mechanisms of astrophysical boundary layers. We focus on the case where the accretion disk extends all… (more)

Subjects/Keywords: accretion; angular momentum; disk; MRI; star; waves

…Density Gap in the Inner Disk and Accretion onto the Star . . . . . . . . . . 160 6.2 Angular… …accretion disk theory. However, there has been surprisingly little work on the dynamics of the… …1978). For B∗ < B∗,crit , the accretion disk will extend all the way to the surface of… …of the disk. If the accretion rate is high enough, it is also possible for material to… …Angular Momentum Transport to Mass Accretion Rate . . . . . . 115 5 Effect of Stratification… 

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APA (6th Edition):

Belyaev, M. (2013). Dynamics of Thin Astrophysical Boundary Layers . (Doctoral Dissertation). Princeton University. Retrieved from http://arks.princeton.edu/ark:/88435/dsp01qn59q405t

Chicago Manual of Style (16th Edition):

Belyaev, Mikhail. “Dynamics of Thin Astrophysical Boundary Layers .” 2013. Doctoral Dissertation, Princeton University. Accessed January 17, 2021. http://arks.princeton.edu/ark:/88435/dsp01qn59q405t.

MLA Handbook (7th Edition):

Belyaev, Mikhail. “Dynamics of Thin Astrophysical Boundary Layers .” 2013. Web. 17 Jan 2021.

Vancouver:

Belyaev M. Dynamics of Thin Astrophysical Boundary Layers . [Internet] [Doctoral dissertation]. Princeton University; 2013. [cited 2021 Jan 17]. Available from: http://arks.princeton.edu/ark:/88435/dsp01qn59q405t.

Council of Science Editors:

Belyaev M. Dynamics of Thin Astrophysical Boundary Layers . [Doctoral Dissertation]. Princeton University; 2013. Available from: http://arks.princeton.edu/ark:/88435/dsp01qn59q405t

17. Rosin, Mark. Instabilities and transport in magnetized plasmas.

Degree: PhD, 2011, University of Cambridge

 In a magnetized plasma, naturally occurring pressure anisotropies facilitate in- stabilities that are expected to modify the transport properties of the system. In this thesis… (more)

Subjects/Keywords: Plasma; Magnetic field; Fluid; Kinetic; Magnetized; Firehose instability; Magnetorotational instatbility; MRI; Transport; Galaxy clusters; Accretion disc; MHD

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APA (6th Edition):

Rosin, M. (2011). Instabilities and transport in magnetized plasmas. (Doctoral Dissertation). University of Cambridge. Retrieved from http://www.dspace.cam.ac.uk/handle/1810/237241https://www.repository.cam.ac.uk/bitstream/1810/237241/2/license.txt ; https://www.repository.cam.ac.uk/bitstream/1810/237241/3/MarkThesis.pdf.txt ; https://www.repository.cam.ac.uk/bitstream/1810/237241/5/MarkThesis.pdf.txt ; https://www.repository.cam.ac.uk/bitstream/1810/237241/6/MarkThesis.pdf.jpg

Chicago Manual of Style (16th Edition):

Rosin, Mark. “Instabilities and transport in magnetized plasmas.” 2011. Doctoral Dissertation, University of Cambridge. Accessed January 17, 2021. http://www.dspace.cam.ac.uk/handle/1810/237241https://www.repository.cam.ac.uk/bitstream/1810/237241/2/license.txt ; https://www.repository.cam.ac.uk/bitstream/1810/237241/3/MarkThesis.pdf.txt ; https://www.repository.cam.ac.uk/bitstream/1810/237241/5/MarkThesis.pdf.txt ; https://www.repository.cam.ac.uk/bitstream/1810/237241/6/MarkThesis.pdf.jpg.

MLA Handbook (7th Edition):

Rosin, Mark. “Instabilities and transport in magnetized plasmas.” 2011. Web. 17 Jan 2021.

Vancouver:

Rosin M. Instabilities and transport in magnetized plasmas. [Internet] [Doctoral dissertation]. University of Cambridge; 2011. [cited 2021 Jan 17]. Available from: http://www.dspace.cam.ac.uk/handle/1810/237241https://www.repository.cam.ac.uk/bitstream/1810/237241/2/license.txt ; https://www.repository.cam.ac.uk/bitstream/1810/237241/3/MarkThesis.pdf.txt ; https://www.repository.cam.ac.uk/bitstream/1810/237241/5/MarkThesis.pdf.txt ; https://www.repository.cam.ac.uk/bitstream/1810/237241/6/MarkThesis.pdf.jpg.

Council of Science Editors:

Rosin M. Instabilities and transport in magnetized plasmas. [Doctoral Dissertation]. University of Cambridge; 2011. Available from: http://www.dspace.cam.ac.uk/handle/1810/237241https://www.repository.cam.ac.uk/bitstream/1810/237241/2/license.txt ; https://www.repository.cam.ac.uk/bitstream/1810/237241/3/MarkThesis.pdf.txt ; https://www.repository.cam.ac.uk/bitstream/1810/237241/5/MarkThesis.pdf.txt ; https://www.repository.cam.ac.uk/bitstream/1810/237241/6/MarkThesis.pdf.jpg


University of Cambridge

18. Rosin, Mark. Instabilities and transport in magnetized plasmas.

Degree: PhD, 2011, University of Cambridge

 In a magnetized plasma, naturally occurring pressure anisotropies facilitate instabilities that are expected to modify the transport properties of the system. In this thesis we… (more)

Subjects/Keywords: 523.01; Plasma; Magnetic field; Fluid; Kinetic; Magnetized; Firehose instability; Magnetorotational instatbility; MRI; Transport; Galaxy clusters; Accretion disc; MHD

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APA (6th Edition):

Rosin, M. (2011). Instabilities and transport in magnetized plasmas. (Doctoral Dissertation). University of Cambridge. Retrieved from https://doi.org/10.17863/CAM.16100 ; https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.541846

Chicago Manual of Style (16th Edition):

Rosin, Mark. “Instabilities and transport in magnetized plasmas.” 2011. Doctoral Dissertation, University of Cambridge. Accessed January 17, 2021. https://doi.org/10.17863/CAM.16100 ; https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.541846.

MLA Handbook (7th Edition):

Rosin, Mark. “Instabilities and transport in magnetized plasmas.” 2011. Web. 17 Jan 2021.

Vancouver:

Rosin M. Instabilities and transport in magnetized plasmas. [Internet] [Doctoral dissertation]. University of Cambridge; 2011. [cited 2021 Jan 17]. Available from: https://doi.org/10.17863/CAM.16100 ; https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.541846.

Council of Science Editors:

Rosin M. Instabilities and transport in magnetized plasmas. [Doctoral Dissertation]. University of Cambridge; 2011. Available from: https://doi.org/10.17863/CAM.16100 ; https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.541846

19. Epitropakis, Anastasios. Variability studies of the iron line emission in AGN.

Degree: 2017, University of Crete (UOC); Πανεπιστήμιο Κρήτης

To this day, the physics and geometry of the inner-most region in active galactic nuclei (AGN) are largely unknown. According to the currently-accepted paradigm, the… (more)

Subjects/Keywords: Δίσκοι προσαύξησης; Ακτίνες-Χ; Σχετικότητα; Ανάλυση δεδομένων; Ανάκτηση δορυφορικών δεδομένων; Ανάλυση δορυφορικών εικόνων; Δορυφορικά δεδομένα; Στατιστικές μέθοδοι; Στατιστικές τεχνικές; Στατιστική βελτιστοποίηση; Αστρονομία; Αστροφυσική; Υπολογιστική αστροφυσική; Accretion; Accretion disc; Accretion disks; X-rays; Relativity; Data analysis; Sattelite data; Statistical analysis; Statistical data analysis; Astronomy; Astrophysics; Computational astrophysics

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APA (6th Edition):

Epitropakis, A. (2017). Variability studies of the iron line emission in AGN. (Thesis). University of Crete (UOC); Πανεπιστήμιο Κρήτης. Retrieved from http://hdl.handle.net/10442/hedi/40954

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Chicago Manual of Style (16th Edition):

Epitropakis, Anastasios. “Variability studies of the iron line emission in AGN.” 2017. Thesis, University of Crete (UOC); Πανεπιστήμιο Κρήτης. Accessed January 17, 2021. http://hdl.handle.net/10442/hedi/40954.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

MLA Handbook (7th Edition):

Epitropakis, Anastasios. “Variability studies of the iron line emission in AGN.” 2017. Web. 17 Jan 2021.

Vancouver:

Epitropakis A. Variability studies of the iron line emission in AGN. [Internet] [Thesis]. University of Crete (UOC); Πανεπιστήμιο Κρήτης; 2017. [cited 2021 Jan 17]. Available from: http://hdl.handle.net/10442/hedi/40954.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Council of Science Editors:

Epitropakis A. Variability studies of the iron line emission in AGN. [Thesis]. University of Crete (UOC); Πανεπιστήμιο Κρήτης; 2017. Available from: http://hdl.handle.net/10442/hedi/40954

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

20. Cridland, Alexander. Connecting the Chemical Composition of Planetary Atmospheres with Planet Formation.

Degree: PhD, 2017, McMaster University

What sets the observable chemical composition of exoplanetary atmospheres? The available chemical abundance of the planet's natal protoplanetary disk gas will have a deciding role… (more)

Subjects/Keywords: Planet formation; Astrochemistry; Accretion disk physics; Dust physics; Planetary atmospheres

…what follows we will discuss the theoretical and observational aspects of accretion disk… …relies on the assumption that the disk is accretion material in what is known as a steady disk… …flow. For a steady disk, Σ has no explicit time dependence, which forces the mass accretion… …evolving accretion disk (LyndenBell & Pringle, 1974) acts as a heating source, and… …Goldreich (1997) derived the midplane temperature and SED for a flared accretion disk… 

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APA (6th Edition):

Cridland, A. (2017). Connecting the Chemical Composition of Planetary Atmospheres with Planet Formation. (Doctoral Dissertation). McMaster University. Retrieved from http://hdl.handle.net/11375/22005

Chicago Manual of Style (16th Edition):

Cridland, Alexander. “Connecting the Chemical Composition of Planetary Atmospheres with Planet Formation.” 2017. Doctoral Dissertation, McMaster University. Accessed January 17, 2021. http://hdl.handle.net/11375/22005.

MLA Handbook (7th Edition):

Cridland, Alexander. “Connecting the Chemical Composition of Planetary Atmospheres with Planet Formation.” 2017. Web. 17 Jan 2021.

Vancouver:

Cridland A. Connecting the Chemical Composition of Planetary Atmospheres with Planet Formation. [Internet] [Doctoral dissertation]. McMaster University; 2017. [cited 2021 Jan 17]. Available from: http://hdl.handle.net/11375/22005.

Council of Science Editors:

Cridland A. Connecting the Chemical Composition of Planetary Atmospheres with Planet Formation. [Doctoral Dissertation]. McMaster University; 2017. Available from: http://hdl.handle.net/11375/22005


McMaster University

21. Hasegawa, Yasuhiro. Planet Traps in Protoplanetary Disks and the Formation and Evolution of Planetary Systems.

Degree: PhD, 2012, McMaster University

  One of the most fundamental problems in theories of planet formation in protoplanetary disks is planetary migration that arises from resonant, tidal interactions of… (more)

Subjects/Keywords: accretion disks; turbulence; planets and satellites: formation; protoplanetary disks; Planet-disk interactions; Astrophysics and Astronomy; Physical Sciences and Mathematics; Astrophysics and Astronomy

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APA (6th Edition):

Hasegawa, Y. (2012). Planet Traps in Protoplanetary Disks and the Formation and Evolution of Planetary Systems. (Doctoral Dissertation). McMaster University. Retrieved from http://hdl.handle.net/11375/12569

Chicago Manual of Style (16th Edition):

Hasegawa, Yasuhiro. “Planet Traps in Protoplanetary Disks and the Formation and Evolution of Planetary Systems.” 2012. Doctoral Dissertation, McMaster University. Accessed January 17, 2021. http://hdl.handle.net/11375/12569.

MLA Handbook (7th Edition):

Hasegawa, Yasuhiro. “Planet Traps in Protoplanetary Disks and the Formation and Evolution of Planetary Systems.” 2012. Web. 17 Jan 2021.

Vancouver:

Hasegawa Y. Planet Traps in Protoplanetary Disks and the Formation and Evolution of Planetary Systems. [Internet] [Doctoral dissertation]. McMaster University; 2012. [cited 2021 Jan 17]. Available from: http://hdl.handle.net/11375/12569.

Council of Science Editors:

Hasegawa Y. Planet Traps in Protoplanetary Disks and the Formation and Evolution of Planetary Systems. [Doctoral Dissertation]. McMaster University; 2012. Available from: http://hdl.handle.net/11375/12569

22. Malmrose, Michael Paul. Thermal emission signatures in non-thermal blazars.

Degree: PhD, Astronomy, 2016, Boston University

 Blazars, a subclass of active galactic nuclei with powerful relativistic plasma jets, are among the most luminous and violently variable objects in the universe. They… (more)

Subjects/Keywords: Astronomy; AGN; Blazars; Dust; Accretion disk; Supermassive black holes

…temperature accretion disk emitting thermal radiation, and 3) an optically thick dusty torus… …wavelengths, radiation originating in the accretion disk. The goal of this study is to determine the… …law Fν ∝ ν −α , and an accretion disk which consists of a thin disk described by the power… …Ray Variability of a Sample of Blazars Compared to Variability of the Accretion Disk 153 6.1… …accretion disk model modified to include a hot blackbody . . . . . . . . . . . . . . . . . . 80… 

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APA (6th Edition):

Malmrose, M. P. (2016). Thermal emission signatures in non-thermal blazars. (Doctoral Dissertation). Boston University. Retrieved from http://hdl.handle.net/2144/19757

Chicago Manual of Style (16th Edition):

Malmrose, Michael Paul. “Thermal emission signatures in non-thermal blazars.” 2016. Doctoral Dissertation, Boston University. Accessed January 17, 2021. http://hdl.handle.net/2144/19757.

MLA Handbook (7th Edition):

Malmrose, Michael Paul. “Thermal emission signatures in non-thermal blazars.” 2016. Web. 17 Jan 2021.

Vancouver:

Malmrose MP. Thermal emission signatures in non-thermal blazars. [Internet] [Doctoral dissertation]. Boston University; 2016. [cited 2021 Jan 17]. Available from: http://hdl.handle.net/2144/19757.

Council of Science Editors:

Malmrose MP. Thermal emission signatures in non-thermal blazars. [Doctoral Dissertation]. Boston University; 2016. Available from: http://hdl.handle.net/2144/19757


George Mason University

23. Makeev, Andrey. Formation of the Power Density Spectrum in the Accreting Compact X-Ray Objects .

Degree: 2010, George Mason University

 One of the remarkable phenomena, characterizing both Galactic and extra-Galactic Xray binary systems, is the substantial variability of a photon ux, detectable in a very… (more)

Subjects/Keywords: accretion disk; power spectrum; x-ray binary; x-ray luminosity; x-ray variability

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APA (6th Edition):

Makeev, A. (2010). Formation of the Power Density Spectrum in the Accreting Compact X-Ray Objects . (Thesis). George Mason University. Retrieved from http://hdl.handle.net/1920/6026

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Chicago Manual of Style (16th Edition):

Makeev, Andrey. “Formation of the Power Density Spectrum in the Accreting Compact X-Ray Objects .” 2010. Thesis, George Mason University. Accessed January 17, 2021. http://hdl.handle.net/1920/6026.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

MLA Handbook (7th Edition):

Makeev, Andrey. “Formation of the Power Density Spectrum in the Accreting Compact X-Ray Objects .” 2010. Web. 17 Jan 2021.

Vancouver:

Makeev A. Formation of the Power Density Spectrum in the Accreting Compact X-Ray Objects . [Internet] [Thesis]. George Mason University; 2010. [cited 2021 Jan 17]. Available from: http://hdl.handle.net/1920/6026.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Council of Science Editors:

Makeev A. Formation of the Power Density Spectrum in the Accreting Compact X-Ray Objects . [Thesis]. George Mason University; 2010. Available from: http://hdl.handle.net/1920/6026

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation


Louisiana State University

24. Megevand, Miguel. Matter sources interacting with a black hole: dynamics and observable signatures.

Degree: PhD, Physical Sciences and Mathematics, 2009, Louisiana State University

 Dynamical systems involving black holes are one of the most promising sources of detectable gravitational waves. Additionally, one expects strong electromagnetic signals whenever matter sources… (more)

Subjects/Keywords: black hole; shocks; kicks; scalar field; galaxy; gravitational waves; accretion disk

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APA (6th Edition):

Megevand, M. (2009). Matter sources interacting with a black hole: dynamics and observable signatures. (Doctoral Dissertation). Louisiana State University. Retrieved from etd-11032009-142431 ; https://digitalcommons.lsu.edu/gradschool_dissertations/2763

Chicago Manual of Style (16th Edition):

Megevand, Miguel. “Matter sources interacting with a black hole: dynamics and observable signatures.” 2009. Doctoral Dissertation, Louisiana State University. Accessed January 17, 2021. etd-11032009-142431 ; https://digitalcommons.lsu.edu/gradschool_dissertations/2763.

MLA Handbook (7th Edition):

Megevand, Miguel. “Matter sources interacting with a black hole: dynamics and observable signatures.” 2009. Web. 17 Jan 2021.

Vancouver:

Megevand M. Matter sources interacting with a black hole: dynamics and observable signatures. [Internet] [Doctoral dissertation]. Louisiana State University; 2009. [cited 2021 Jan 17]. Available from: etd-11032009-142431 ; https://digitalcommons.lsu.edu/gradschool_dissertations/2763.

Council of Science Editors:

Megevand M. Matter sources interacting with a black hole: dynamics and observable signatures. [Doctoral Dissertation]. Louisiana State University; 2009. Available from: etd-11032009-142431 ; https://digitalcommons.lsu.edu/gradschool_dissertations/2763

25. Schilbach, Tyson. Accretion Disk Contributions to the Diffuse Neutrino Background.

Degree: MS, Department of Physics, 2018, University of Guelph

 Predictions for AD neutrino detection at Super Kamiokande and Hyper Kamiokande are made. Concepts related to the diffuse neutrino background for accretion disks are introduced.… (more)

Subjects/Keywords: Physics; Nuclear; Astrophysics; Neutrino; Diffuse Background; Accretion Disk

…work will focus on three accretion disk sources. Neutron star - neutron star mergers, black… …accretion disk neutrinos as it is already calibrated for supernova neutrinos. The primary range of… …neutrino spectra for a single accretion disk is reviewed. From here, two red shifts are… …detection in a Earth-based water Cherenkov detector can be found. 2.1 Disk Models Accretion… …thermodynamical properties of the accretion disk relative to distance from the black hole. The model… 

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APA (6th Edition):

Schilbach, T. (2018). Accretion Disk Contributions to the Diffuse Neutrino Background. (Masters Thesis). University of Guelph. Retrieved from https://atrium.lib.uoguelph.ca/xmlui/handle/10214/14280

Chicago Manual of Style (16th Edition):

Schilbach, Tyson. “Accretion Disk Contributions to the Diffuse Neutrino Background.” 2018. Masters Thesis, University of Guelph. Accessed January 17, 2021. https://atrium.lib.uoguelph.ca/xmlui/handle/10214/14280.

MLA Handbook (7th Edition):

Schilbach, Tyson. “Accretion Disk Contributions to the Diffuse Neutrino Background.” 2018. Web. 17 Jan 2021.

Vancouver:

Schilbach T. Accretion Disk Contributions to the Diffuse Neutrino Background. [Internet] [Masters thesis]. University of Guelph; 2018. [cited 2021 Jan 17]. Available from: https://atrium.lib.uoguelph.ca/xmlui/handle/10214/14280.

Council of Science Editors:

Schilbach T. Accretion Disk Contributions to the Diffuse Neutrino Background. [Masters Thesis]. University of Guelph; 2018. Available from: https://atrium.lib.uoguelph.ca/xmlui/handle/10214/14280

26. Isogai, Keisuke. Observational Research on Dwarf Novae: Superoutburst, Evolution, and Development of a Classification Method Using Gaia DR2 .

Degree: 2019, Kyoto University

Subjects/Keywords: accretion disk; cataclysmic variable; dwarf nova; superoutburst; AM CVn star

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APA (6th Edition):

Isogai, K. (2019). Observational Research on Dwarf Novae: Superoutburst, Evolution, and Development of a Classification Method Using Gaia DR2 . (Thesis). Kyoto University. Retrieved from http://hdl.handle.net/2433/242610

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Chicago Manual of Style (16th Edition):

Isogai, Keisuke. “Observational Research on Dwarf Novae: Superoutburst, Evolution, and Development of a Classification Method Using Gaia DR2 .” 2019. Thesis, Kyoto University. Accessed January 17, 2021. http://hdl.handle.net/2433/242610.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

MLA Handbook (7th Edition):

Isogai, Keisuke. “Observational Research on Dwarf Novae: Superoutburst, Evolution, and Development of a Classification Method Using Gaia DR2 .” 2019. Web. 17 Jan 2021.

Vancouver:

Isogai K. Observational Research on Dwarf Novae: Superoutburst, Evolution, and Development of a Classification Method Using Gaia DR2 . [Internet] [Thesis]. Kyoto University; 2019. [cited 2021 Jan 17]. Available from: http://hdl.handle.net/2433/242610.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Council of Science Editors:

Isogai K. Observational Research on Dwarf Novae: Superoutburst, Evolution, and Development of a Classification Method Using Gaia DR2 . [Thesis]. Kyoto University; 2019. Available from: http://hdl.handle.net/2433/242610

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation


The Ohio State University

27. Poindexter, Shawn David. Sharpening The Tools of Gravitational Microlensing.

Degree: PhD, Astronomy, 2009, The Ohio State University

  We attempt to identify all microlensing parallax events for which the parallax fit improves ΔΧ2 > 100 relative to a standard microlensing model. We… (more)

Subjects/Keywords: Astronomy; gravitational lensing; microlensing; parallax; xallarap; quasar microlensing; accretion disk

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APA · Chicago · MLA · Vancouver · CSE | Export to Zotero / EndNote / Reference Manager

APA (6th Edition):

Poindexter, S. D. (2009). Sharpening The Tools of Gravitational Microlensing. (Doctoral Dissertation). The Ohio State University. Retrieved from http://rave.ohiolink.edu/etdc/view?acc_num=osu1258766992

Chicago Manual of Style (16th Edition):

Poindexter, Shawn David. “Sharpening The Tools of Gravitational Microlensing.” 2009. Doctoral Dissertation, The Ohio State University. Accessed January 17, 2021. http://rave.ohiolink.edu/etdc/view?acc_num=osu1258766992.

MLA Handbook (7th Edition):

Poindexter, Shawn David. “Sharpening The Tools of Gravitational Microlensing.” 2009. Web. 17 Jan 2021.

Vancouver:

Poindexter SD. Sharpening The Tools of Gravitational Microlensing. [Internet] [Doctoral dissertation]. The Ohio State University; 2009. [cited 2021 Jan 17]. Available from: http://rave.ohiolink.edu/etdc/view?acc_num=osu1258766992.

Council of Science Editors:

Poindexter SD. Sharpening The Tools of Gravitational Microlensing. [Doctoral Dissertation]. The Ohio State University; 2009. Available from: http://rave.ohiolink.edu/etdc/view?acc_num=osu1258766992


University of Texas – Austin

28. Bayless, Amanda Jo. Accretion disks in low-mass X-ray binaries in ultraviolet and optical wavelengths.

Degree: PhD, Astronomy, 2010, University of Texas – Austin

 We present new models for two low-mass X-ray binaries (LMXB), 4U 1822-371 and V1408 Aql (= 4U 1957+115). The eclipsing LMXB 4U 1822-371 is the… (more)

Subjects/Keywords: X-ray binaries; Eclipsing binaries; Compact objects; Accretion disk corona

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APA · Chicago · MLA · Vancouver · CSE | Export to Zotero / EndNote / Reference Manager

APA (6th Edition):

Bayless, A. J. (2010). Accretion disks in low-mass X-ray binaries in ultraviolet and optical wavelengths. (Doctoral Dissertation). University of Texas – Austin. Retrieved from http://hdl.handle.net/2152/ETD-UT-2010-08-1727

Chicago Manual of Style (16th Edition):

Bayless, Amanda Jo. “Accretion disks in low-mass X-ray binaries in ultraviolet and optical wavelengths.” 2010. Doctoral Dissertation, University of Texas – Austin. Accessed January 17, 2021. http://hdl.handle.net/2152/ETD-UT-2010-08-1727.

MLA Handbook (7th Edition):

Bayless, Amanda Jo. “Accretion disks in low-mass X-ray binaries in ultraviolet and optical wavelengths.” 2010. Web. 17 Jan 2021.

Vancouver:

Bayless AJ. Accretion disks in low-mass X-ray binaries in ultraviolet and optical wavelengths. [Internet] [Doctoral dissertation]. University of Texas – Austin; 2010. [cited 2021 Jan 17]. Available from: http://hdl.handle.net/2152/ETD-UT-2010-08-1727.

Council of Science Editors:

Bayless AJ. Accretion disks in low-mass X-ray binaries in ultraviolet and optical wavelengths. [Doctoral Dissertation]. University of Texas – Austin; 2010. Available from: http://hdl.handle.net/2152/ETD-UT-2010-08-1727

29. Nauta, Michiel Doede. Two-dimensional vortices and accretion disks.

Degree: 2000, University Utrecht

 Observations show that there are disks around certain stars that slowly rain down on the central (compact) object: accretion disks. The rate of depletion of… (more)

Subjects/Keywords: accretion disk; VORTEX; geophysical fluid dynamics; two-dimensional turbulence; shocks; angular momentum transport

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APA · Chicago · MLA · Vancouver · CSE | Export to Zotero / EndNote / Reference Manager

APA (6th Edition):

Nauta, M. D. (2000). Two-dimensional vortices and accretion disks. (Doctoral Dissertation). University Utrecht. Retrieved from https://dspace.library.uu.nl/handle/1874/639 ; URN:NBN:NL:UI:10-1874-639 ; 1874/639 ; URN:NBN:NL:UI:10-1874-639 ; https://dspace.library.uu.nl/handle/1874/639

Chicago Manual of Style (16th Edition):

Nauta, Michiel Doede. “Two-dimensional vortices and accretion disks.” 2000. Doctoral Dissertation, University Utrecht. Accessed January 17, 2021. https://dspace.library.uu.nl/handle/1874/639 ; URN:NBN:NL:UI:10-1874-639 ; 1874/639 ; URN:NBN:NL:UI:10-1874-639 ; https://dspace.library.uu.nl/handle/1874/639.

MLA Handbook (7th Edition):

Nauta, Michiel Doede. “Two-dimensional vortices and accretion disks.” 2000. Web. 17 Jan 2021.

Vancouver:

Nauta MD. Two-dimensional vortices and accretion disks. [Internet] [Doctoral dissertation]. University Utrecht; 2000. [cited 2021 Jan 17]. Available from: https://dspace.library.uu.nl/handle/1874/639 ; URN:NBN:NL:UI:10-1874-639 ; 1874/639 ; URN:NBN:NL:UI:10-1874-639 ; https://dspace.library.uu.nl/handle/1874/639.

Council of Science Editors:

Nauta MD. Two-dimensional vortices and accretion disks. [Doctoral Dissertation]. University Utrecht; 2000. Available from: https://dspace.library.uu.nl/handle/1874/639 ; URN:NBN:NL:UI:10-1874-639 ; 1874/639 ; URN:NBN:NL:UI:10-1874-639 ; https://dspace.library.uu.nl/handle/1874/639

30. E. Ragusa. THE EVOLUTION OF BINARY SYSTEMS IN GASEOUS ENVIRONMENTS.

Degree: 2018, Università degli Studi di Milano

 Systems where a binary, that is two gravitationally bound objects orbiting their centre of mass, interacts with the surrounding gas or dust are extremely common… (more)

Subjects/Keywords: Protoplanetary discs; Planet formation; Black hole binaries; Satellite-disc interaction; Accretion discs; satellite migration; eccentricity evolution; non-axisymmetric features; Settore FIS/05 - Astronomia e Astrofisica

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APA · Chicago · MLA · Vancouver · CSE | Export to Zotero / EndNote / Reference Manager

APA (6th Edition):

Ragusa, E. (2018). THE EVOLUTION OF BINARY SYSTEMS IN GASEOUS ENVIRONMENTS. (Thesis). Università degli Studi di Milano. Retrieved from http://hdl.handle.net/2434/604177

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Chicago Manual of Style (16th Edition):

Ragusa, E.. “THE EVOLUTION OF BINARY SYSTEMS IN GASEOUS ENVIRONMENTS.” 2018. Thesis, Università degli Studi di Milano. Accessed January 17, 2021. http://hdl.handle.net/2434/604177.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

MLA Handbook (7th Edition):

Ragusa, E.. “THE EVOLUTION OF BINARY SYSTEMS IN GASEOUS ENVIRONMENTS.” 2018. Web. 17 Jan 2021.

Vancouver:

Ragusa E. THE EVOLUTION OF BINARY SYSTEMS IN GASEOUS ENVIRONMENTS. [Internet] [Thesis]. Università degli Studi di Milano; 2018. [cited 2021 Jan 17]. Available from: http://hdl.handle.net/2434/604177.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Council of Science Editors:

Ragusa E. THE EVOLUTION OF BINARY SYSTEMS IN GASEOUS ENVIRONMENTS. [Thesis]. Università degli Studi di Milano; 2018. Available from: http://hdl.handle.net/2434/604177

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

[1] [2]

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