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You searched for subject:(Accretion Disks). Showing records 1 – 30 of 84 total matches.

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Clemson University

1. Speights, Christa. Star-Disk Interaction in Herbig Ae/Be Stars.

Degree: MS, Astrophysics, 2012, Clemson University

 The question of the mechanism of certain types of stars is important. Classical T Tauri (CTTS) stars accrete magnetospherically, and Herbig Ae/Be stars (higher-mass analogs… (more)

Subjects/Keywords: accretion; accretion disks; Astrophysics and Astronomy

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APA (6th Edition):

Speights, C. (2012). Star-Disk Interaction in Herbig Ae/Be Stars. (Masters Thesis). Clemson University. Retrieved from https://tigerprints.clemson.edu/all_theses/1476

Chicago Manual of Style (16th Edition):

Speights, Christa. “Star-Disk Interaction in Herbig Ae/Be Stars.” 2012. Masters Thesis, Clemson University. Accessed July 20, 2019. https://tigerprints.clemson.edu/all_theses/1476.

MLA Handbook (7th Edition):

Speights, Christa. “Star-Disk Interaction in Herbig Ae/Be Stars.” 2012. Web. 20 Jul 2019.

Vancouver:

Speights C. Star-Disk Interaction in Herbig Ae/Be Stars. [Internet] [Masters thesis]. Clemson University; 2012. [cited 2019 Jul 20]. Available from: https://tigerprints.clemson.edu/all_theses/1476.

Council of Science Editors:

Speights C. Star-Disk Interaction in Herbig Ae/Be Stars. [Masters Thesis]. Clemson University; 2012. Available from: https://tigerprints.clemson.edu/all_theses/1476


Cornell University

2. Long, Min. Disk Accretion to Rotating Magnetized Stars: Magnetohydrodynamic Simulations .

Degree: 2008, Cornell University

 The star-disk interaction between a rotating magnetized star and a surrounding accretion disk is a fundamental process in astrophysics, and is usually difficult to investigate… (more)

Subjects/Keywords: accretion; accretion disks; magnetic fields; magnetohydrodynamics

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APA (6th Edition):

Long, M. (2008). Disk Accretion to Rotating Magnetized Stars: Magnetohydrodynamic Simulations . (Thesis). Cornell University. Retrieved from http://hdl.handle.net/1813/10759

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):

Long, Min. “Disk Accretion to Rotating Magnetized Stars: Magnetohydrodynamic Simulations .” 2008. Thesis, Cornell University. Accessed July 20, 2019. http://hdl.handle.net/1813/10759.

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

MLA Handbook (7th Edition):

Long, Min. “Disk Accretion to Rotating Magnetized Stars: Magnetohydrodynamic Simulations .” 2008. Web. 20 Jul 2019.

Vancouver:

Long M. Disk Accretion to Rotating Magnetized Stars: Magnetohydrodynamic Simulations . [Internet] [Thesis]. Cornell University; 2008. [cited 2019 Jul 20]. Available from: http://hdl.handle.net/1813/10759.

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

Council of Science Editors:

Long M. Disk Accretion to Rotating Magnetized Stars: Magnetohydrodynamic Simulations . [Thesis]. Cornell University; 2008. Available from: http://hdl.handle.net/1813/10759

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


Cornell University

3. Lii, Patrick. Outflows And Accretion At The Disk-Magnetosphere Boundary .

Degree: 2015, Cornell University

 Accreting magnetized stars are ubiquitous throughout astrophysics and can be found in a variety of astrophysical contexts at both the dawning and closing stages of… (more)

Subjects/Keywords: accretion disks; magnetohydrodynamics; young stellar objects

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APA (6th Edition):

Lii, P. (2015). Outflows And Accretion At The Disk-Magnetosphere Boundary . (Thesis). Cornell University. Retrieved from http://hdl.handle.net/1813/41001

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):

Lii, Patrick. “Outflows And Accretion At The Disk-Magnetosphere Boundary .” 2015. Thesis, Cornell University. Accessed July 20, 2019. http://hdl.handle.net/1813/41001.

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

MLA Handbook (7th Edition):

Lii, Patrick. “Outflows And Accretion At The Disk-Magnetosphere Boundary .” 2015. Web. 20 Jul 2019.

Vancouver:

Lii P. Outflows And Accretion At The Disk-Magnetosphere Boundary . [Internet] [Thesis]. Cornell University; 2015. [cited 2019 Jul 20]. Available from: http://hdl.handle.net/1813/41001.

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

Council of Science Editors:

Lii P. Outflows And Accretion At The Disk-Magnetosphere Boundary . [Thesis]. Cornell University; 2015. Available from: http://hdl.handle.net/1813/41001

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


Princeton University

4. Ju, Wenhua. Magnetohydrodynamics of Accretion Disks in Cataclysmic Variables .

Degree: PhD, 2016, Princeton University

 Angular momentum transport in the accretion disks of cataclysmic variables (CVs) is a crucial ingredient of driving the evolution of CVs and is believed to… (more)

Subjects/Keywords: accretion disks; cataclysmic variable; dwarf novae; magnetohydrodynamics

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APA (6th Edition):

Ju, W. (2016). Magnetohydrodynamics of Accretion Disks in Cataclysmic Variables . (Doctoral Dissertation). Princeton University. Retrieved from http://arks.princeton.edu/ark:/88435/dsp017s75df84b

Chicago Manual of Style (16th Edition):

Ju, Wenhua. “Magnetohydrodynamics of Accretion Disks in Cataclysmic Variables .” 2016. Doctoral Dissertation, Princeton University. Accessed July 20, 2019. http://arks.princeton.edu/ark:/88435/dsp017s75df84b.

MLA Handbook (7th Edition):

Ju, Wenhua. “Magnetohydrodynamics of Accretion Disks in Cataclysmic Variables .” 2016. Web. 20 Jul 2019.

Vancouver:

Ju W. Magnetohydrodynamics of Accretion Disks in Cataclysmic Variables . [Internet] [Doctoral dissertation]. Princeton University; 2016. [cited 2019 Jul 20]. Available from: http://arks.princeton.edu/ark:/88435/dsp017s75df84b.

Council of Science Editors:

Ju W. Magnetohydrodynamics of Accretion Disks in Cataclysmic Variables . [Doctoral Dissertation]. Princeton University; 2016. Available from: http://arks.princeton.edu/ark:/88435/dsp017s75df84b


Cornell University

5. Miranda, Ryan Joseph. Hydrodynamical Processes in Astrophysical Disks .

Degree: 2017, Cornell University

Accretion disks – distributions of gas orbiting a central massive object – are found in a variety of astrophysical settings, such as protoplanetary disks around young stars… (more)

Subjects/Keywords: Astrophysics; accretion disks; astrophysical fluid dynamics; Astronomy

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APA (6th Edition):

Miranda, R. J. (2017). Hydrodynamical Processes in Astrophysical Disks . (Thesis). Cornell University. Retrieved from http://hdl.handle.net/1813/59144

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):

Miranda, Ryan Joseph. “Hydrodynamical Processes in Astrophysical Disks .” 2017. Thesis, Cornell University. Accessed July 20, 2019. http://hdl.handle.net/1813/59144.

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

MLA Handbook (7th Edition):

Miranda, Ryan Joseph. “Hydrodynamical Processes in Astrophysical Disks .” 2017. Web. 20 Jul 2019.

Vancouver:

Miranda RJ. Hydrodynamical Processes in Astrophysical Disks . [Internet] [Thesis]. Cornell University; 2017. [cited 2019 Jul 20]. Available from: http://hdl.handle.net/1813/59144.

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

Council of Science Editors:

Miranda RJ. Hydrodynamical Processes in Astrophysical Disks . [Thesis]. Cornell University; 2017. Available from: http://hdl.handle.net/1813/59144

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


The Ohio State University

6. Morgan, Christopher Warren. Quasar Structure from Microlensing in Gravitationally Lensed Quasars.

Degree: PhD, Astronomy, 2008, The Ohio State University

  I analyze microlensing in gravitationally lensed quasars to yield measurements of the structure of their continuum emission regions. I first describe our lensed quasar… (more)

Subjects/Keywords: Astronomy; Astrophysics; accretion, accretion disks; dark matter; gravitational lensing; quasars: general

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APA (6th Edition):

Morgan, C. W. (2008). Quasar Structure from Microlensing in Gravitationally Lensed Quasars. (Doctoral Dissertation). The Ohio State University. Retrieved from http://rave.ohiolink.edu/etdc/view?acc_num=osu1205848751

Chicago Manual of Style (16th Edition):

Morgan, Christopher Warren. “Quasar Structure from Microlensing in Gravitationally Lensed Quasars.” 2008. Doctoral Dissertation, The Ohio State University. Accessed July 20, 2019. http://rave.ohiolink.edu/etdc/view?acc_num=osu1205848751.

MLA Handbook (7th Edition):

Morgan, Christopher Warren. “Quasar Structure from Microlensing in Gravitationally Lensed Quasars.” 2008. Web. 20 Jul 2019.

Vancouver:

Morgan CW. Quasar Structure from Microlensing in Gravitationally Lensed Quasars. [Internet] [Doctoral dissertation]. The Ohio State University; 2008. [cited 2019 Jul 20]. Available from: http://rave.ohiolink.edu/etdc/view?acc_num=osu1205848751.

Council of Science Editors:

Morgan CW. Quasar Structure from Microlensing in Gravitationally Lensed Quasars. [Doctoral Dissertation]. The Ohio State University; 2008. Available from: http://rave.ohiolink.edu/etdc/view?acc_num=osu1205848751


University of Texas – Austin

7. Yu, Mo, Ph. D. Probing giant-planet forming zones around Solar-like stars with CO.

Degree: Astronomy, 2017, University of Texas – Austin

 Protoplanetary disks are dusty disks around young stars where planets are formed. The evolution and composition of protoplanetary disks determine the time, environments and materials… (more)

Subjects/Keywords: Protoplanetary disks; Planet formation; Astrochemistry; Molecular line profiles; Accretion disks; Turbulence

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APA (6th Edition):

Yu, Mo, P. D. (2017). Probing giant-planet forming zones around Solar-like stars with CO. (Thesis). University of Texas – Austin. Retrieved from http://hdl.handle.net/2152/61889

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):

Yu, Mo, Ph D. “Probing giant-planet forming zones around Solar-like stars with CO.” 2017. Thesis, University of Texas – Austin. Accessed July 20, 2019. http://hdl.handle.net/2152/61889.

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

MLA Handbook (7th Edition):

Yu, Mo, Ph D. “Probing giant-planet forming zones around Solar-like stars with CO.” 2017. Web. 20 Jul 2019.

Vancouver:

Yu, Mo PD. Probing giant-planet forming zones around Solar-like stars with CO. [Internet] [Thesis]. University of Texas – Austin; 2017. [cited 2019 Jul 20]. Available from: http://hdl.handle.net/2152/61889.

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

Council of Science Editors:

Yu, Mo PD. Probing giant-planet forming zones around Solar-like stars with CO. [Thesis]. University of Texas – Austin; 2017. Available from: http://hdl.handle.net/2152/61889

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


University of Cambridge

8. Vanon, Riccardo. Zonal flows in accretion discs and their role in gravito-turbulence .

Degree: 2017, University of Cambridge

 This thesis focuses on the evolution of zonal flows in self-gravitating accretion discs and their resulting effect on disc stability; it also studies the process… (more)

Subjects/Keywords: accretion; accretion discs; accretion disks; accretion flow; turbulence; astrophysics; astronomy; astrophysical fluid dynamics; fluid dynamics; computational fluid dynamics; cfd; spectral methods; C; fluid mechanics; protoplanetary discs; protoplanetary disks; agns; galaxies

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APA (6th Edition):

Vanon, R. (2017). Zonal flows in accretion discs and their role in gravito-turbulence . (Thesis). University of Cambridge. Retrieved from https://www.repository.cam.ac.uk/handle/1810/267991

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):

Vanon, Riccardo. “Zonal flows in accretion discs and their role in gravito-turbulence .” 2017. Thesis, University of Cambridge. Accessed July 20, 2019. https://www.repository.cam.ac.uk/handle/1810/267991.

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

MLA Handbook (7th Edition):

Vanon, Riccardo. “Zonal flows in accretion discs and their role in gravito-turbulence .” 2017. Web. 20 Jul 2019.

Vancouver:

Vanon R. Zonal flows in accretion discs and their role in gravito-turbulence . [Internet] [Thesis]. University of Cambridge; 2017. [cited 2019 Jul 20]. Available from: https://www.repository.cam.ac.uk/handle/1810/267991.

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

Council of Science Editors:

Vanon R. Zonal flows in accretion discs and their role in gravito-turbulence . [Thesis]. University of Cambridge; 2017. Available from: https://www.repository.cam.ac.uk/handle/1810/267991

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


University of Texas – Austin

9. Lindner, Christopher Carl. Collapsar accretion and the gamma-ray burst X-ray light curve.

Degree: Astronomy, 2010, University of Texas – Austin

 We present axisymmetric hydrodynamical simulations of the long-term accretion of a rotating gamma-ray burst progenitor star, a "collapsar," onto the central compact object, which we… (more)

Subjects/Keywords: Accretion; Accretion disks; Black hole physics; Gamma-ray bursts; Winds; Outflows; Supernovae

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APA (6th Edition):

Lindner, C. C. (2010). Collapsar accretion and the gamma-ray burst X-ray light curve. (Thesis). University of Texas – Austin. Retrieved from http://hdl.handle.net/2152/ETD-UT-2010-05-1431

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):

Lindner, Christopher Carl. “Collapsar accretion and the gamma-ray burst X-ray light curve.” 2010. Thesis, University of Texas – Austin. Accessed July 20, 2019. http://hdl.handle.net/2152/ETD-UT-2010-05-1431.

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

MLA Handbook (7th Edition):

Lindner, Christopher Carl. “Collapsar accretion and the gamma-ray burst X-ray light curve.” 2010. Web. 20 Jul 2019.

Vancouver:

Lindner CC. Collapsar accretion and the gamma-ray burst X-ray light curve. [Internet] [Thesis]. University of Texas – Austin; 2010. [cited 2019 Jul 20]. Available from: http://hdl.handle.net/2152/ETD-UT-2010-05-1431.

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

Council of Science Editors:

Lindner CC. Collapsar accretion and the gamma-ray burst X-ray light curve. [Thesis]. University of Texas – Austin; 2010. Available from: http://hdl.handle.net/2152/ETD-UT-2010-05-1431

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


Princeton University

10. Wang, Lile. Simulating Dispersal of Protoplanetary Disks and Planetary Atmospheres with Consistent Radiation and Thermochemistry .

Degree: PhD, 2018, Princeton University

 This thesis focuses on combining (magneto-)hydrodynamic (HD/MHD) simulations with consistent radiation and thermochemistry. We implement a simulation code, an extensions of the Godunov HD/MHD solver… (more)

Subjects/Keywords: accretion; accretion disks; circunstellar matter; magnetohydrodynamics (MHD); method:numerical; planets and satellites: formation

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APA (6th Edition):

Wang, L. (2018). Simulating Dispersal of Protoplanetary Disks and Planetary Atmospheres with Consistent Radiation and Thermochemistry . (Doctoral Dissertation). Princeton University. Retrieved from http://arks.princeton.edu/ark:/88435/dsp013t945t53n

Chicago Manual of Style (16th Edition):

Wang, Lile. “Simulating Dispersal of Protoplanetary Disks and Planetary Atmospheres with Consistent Radiation and Thermochemistry .” 2018. Doctoral Dissertation, Princeton University. Accessed July 20, 2019. http://arks.princeton.edu/ark:/88435/dsp013t945t53n.

MLA Handbook (7th Edition):

Wang, Lile. “Simulating Dispersal of Protoplanetary Disks and Planetary Atmospheres with Consistent Radiation and Thermochemistry .” 2018. Web. 20 Jul 2019.

Vancouver:

Wang L. Simulating Dispersal of Protoplanetary Disks and Planetary Atmospheres with Consistent Radiation and Thermochemistry . [Internet] [Doctoral dissertation]. Princeton University; 2018. [cited 2019 Jul 20]. Available from: http://arks.princeton.edu/ark:/88435/dsp013t945t53n.

Council of Science Editors:

Wang L. Simulating Dispersal of Protoplanetary Disks and Planetary Atmospheres with Consistent Radiation and Thermochemistry . [Doctoral Dissertation]. Princeton University; 2018. Available from: http://arks.princeton.edu/ark:/88435/dsp013t945t53n


Rochester Institute of Technology

11. Bowen, Dennis B. General Relativistic Gas Dynamics in the Central Cavity of Binary Black Holes.

Degree: PhD, School of Physics and Astronomy (COS), 2017, Rochester Institute of Technology

  Supermassive binary black holes (SMBBHs) represent an excellent candidate for future combined gravitational wave and electromagnetic astrophysics, commonly referred to as multimessenger astrophysics. While… (more)

Subjects/Keywords: Accretion; Accretion disks; Binary black hole; Black hole physics; General relativity; Magnetohydrodynamics

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APA (6th Edition):

Bowen, D. B. (2017). General Relativistic Gas Dynamics in the Central Cavity of Binary Black Holes. (Doctoral Dissertation). Rochester Institute of Technology. Retrieved from https://scholarworks.rit.edu/theses/9604

Chicago Manual of Style (16th Edition):

Bowen, Dennis B. “General Relativistic Gas Dynamics in the Central Cavity of Binary Black Holes.” 2017. Doctoral Dissertation, Rochester Institute of Technology. Accessed July 20, 2019. https://scholarworks.rit.edu/theses/9604.

MLA Handbook (7th Edition):

Bowen, Dennis B. “General Relativistic Gas Dynamics in the Central Cavity of Binary Black Holes.” 2017. Web. 20 Jul 2019.

Vancouver:

Bowen DB. General Relativistic Gas Dynamics in the Central Cavity of Binary Black Holes. [Internet] [Doctoral dissertation]. Rochester Institute of Technology; 2017. [cited 2019 Jul 20]. Available from: https://scholarworks.rit.edu/theses/9604.

Council of Science Editors:

Bowen DB. General Relativistic Gas Dynamics in the Central Cavity of Binary Black Holes. [Doctoral Dissertation]. Rochester Institute of Technology; 2017. Available from: https://scholarworks.rit.edu/theses/9604


University of Arizona

12. Johannsen, Tim. Testing General Relativity in the Strong-Field Regime with Observations of Black Holes in the Electromagnetic Spectrum .

Degree: 2012, University of Arizona

 General relativity has been tested by many experiments, which, however, almost exclusively probe weak spacetime curvatures. In this thesis, I create two frameworks for testing… (more)

Subjects/Keywords: black hole physics; galaxy; center; gravitation; relativistic processes; X-rays; binaries; Physics; accretion; accretion disks

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APA (6th Edition):

Johannsen, T. (2012). Testing General Relativity in the Strong-Field Regime with Observations of Black Holes in the Electromagnetic Spectrum . (Doctoral Dissertation). University of Arizona. Retrieved from http://hdl.handle.net/10150/238893

Chicago Manual of Style (16th Edition):

Johannsen, Tim. “Testing General Relativity in the Strong-Field Regime with Observations of Black Holes in the Electromagnetic Spectrum .” 2012. Doctoral Dissertation, University of Arizona. Accessed July 20, 2019. http://hdl.handle.net/10150/238893.

MLA Handbook (7th Edition):

Johannsen, Tim. “Testing General Relativity in the Strong-Field Regime with Observations of Black Holes in the Electromagnetic Spectrum .” 2012. Web. 20 Jul 2019.

Vancouver:

Johannsen T. Testing General Relativity in the Strong-Field Regime with Observations of Black Holes in the Electromagnetic Spectrum . [Internet] [Doctoral dissertation]. University of Arizona; 2012. [cited 2019 Jul 20]. Available from: http://hdl.handle.net/10150/238893.

Council of Science Editors:

Johannsen T. Testing General Relativity in the Strong-Field Regime with Observations of Black Holes in the Electromagnetic Spectrum . [Doctoral Dissertation]. University of Arizona; 2012. Available from: http://hdl.handle.net/10150/238893


Louisiana State University

13. Korobkin, Oleg. Non-axisymmetric instabilities in self-gravitating tori around black holes, and solving Einstein constraints with superconvergent finite element methods.

Degree: PhD, Physical Sciences and Mathematics, 2010, Louisiana State University

 This thesis contains results on two related projects. In the first project, we explore non-axisymmetric instabilities in general relativistic accretion disks around black holes. Such… (more)

Subjects/Keywords: black holes; accretion disks; self-gravitating disks; gamma-ray burst central engines; multiblock approach

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APA (6th Edition):

Korobkin, O. (2010). Non-axisymmetric instabilities in self-gravitating tori around black holes, and solving Einstein constraints with superconvergent finite element methods. (Doctoral Dissertation). Louisiana State University. Retrieved from etd-11122010-153530 ; https://digitalcommons.lsu.edu/gradschool_dissertations/3666

Chicago Manual of Style (16th Edition):

Korobkin, Oleg. “Non-axisymmetric instabilities in self-gravitating tori around black holes, and solving Einstein constraints with superconvergent finite element methods.” 2010. Doctoral Dissertation, Louisiana State University. Accessed July 20, 2019. etd-11122010-153530 ; https://digitalcommons.lsu.edu/gradschool_dissertations/3666.

MLA Handbook (7th Edition):

Korobkin, Oleg. “Non-axisymmetric instabilities in self-gravitating tori around black holes, and solving Einstein constraints with superconvergent finite element methods.” 2010. Web. 20 Jul 2019.

Vancouver:

Korobkin O. Non-axisymmetric instabilities in self-gravitating tori around black holes, and solving Einstein constraints with superconvergent finite element methods. [Internet] [Doctoral dissertation]. Louisiana State University; 2010. [cited 2019 Jul 20]. Available from: etd-11122010-153530 ; https://digitalcommons.lsu.edu/gradschool_dissertations/3666.

Council of Science Editors:

Korobkin O. Non-axisymmetric instabilities in self-gravitating tori around black holes, and solving Einstein constraints with superconvergent finite element methods. [Doctoral Dissertation]. Louisiana State University; 2010. Available from: etd-11122010-153530 ; https://digitalcommons.lsu.edu/gradschool_dissertations/3666


University of Illinois – Urbana-Champaign

14. Yang, Chao-Chin. Planetesimal and Protoplanet Dynamics in a Turbulent Protoplanetary Disk.

Degree: PhD, 0333, 2010, University of Illinois – Urbana-Champaign

 In a young protoplanetary disk, planetary objects undergo orbital migration due to the gravitational torques exerted by their surrounding gas. It has been an outstanding… (more)

Subjects/Keywords: Accretion Disks; Instabilities; Numerical methods; Magnetohydrodynamics (MHD); Planetary systems: formation; Protoplanetary disks; Turbulence

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APA (6th Edition):

Yang, C. (2010). Planetesimal and Protoplanet Dynamics in a Turbulent Protoplanetary Disk. (Doctoral Dissertation). University of Illinois – Urbana-Champaign. Retrieved from http://hdl.handle.net/2142/17009

Chicago Manual of Style (16th Edition):

Yang, Chao-Chin. “Planetesimal and Protoplanet Dynamics in a Turbulent Protoplanetary Disk.” 2010. Doctoral Dissertation, University of Illinois – Urbana-Champaign. Accessed July 20, 2019. http://hdl.handle.net/2142/17009.

MLA Handbook (7th Edition):

Yang, Chao-Chin. “Planetesimal and Protoplanet Dynamics in a Turbulent Protoplanetary Disk.” 2010. Web. 20 Jul 2019.

Vancouver:

Yang C. Planetesimal and Protoplanet Dynamics in a Turbulent Protoplanetary Disk. [Internet] [Doctoral dissertation]. University of Illinois – Urbana-Champaign; 2010. [cited 2019 Jul 20]. Available from: http://hdl.handle.net/2142/17009.

Council of Science Editors:

Yang C. Planetesimal and Protoplanet Dynamics in a Turbulent Protoplanetary Disk. [Doctoral Dissertation]. University of Illinois – Urbana-Champaign; 2010. Available from: http://hdl.handle.net/2142/17009


University of Colorado

15. Hughes, Anna Louise Haugsjaa. Mixing of Dust in Protoplanetary Disks and the Solar Nebula.

Degree: PhD, Astrophysical & Planetary Sciences, 2011, University of Colorado

  Understanding the small-dust component of protoplanetary disks is key to understanding the conditions for planet formation. Small dust grains, particularly at large distances, provide… (more)

Subjects/Keywords: accretion; aerodynamics; comets; dust; planetesimals; protoplanetary disks; Astrophysics and Astronomy

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APA (6th Edition):

Hughes, A. L. H. (2011). Mixing of Dust in Protoplanetary Disks and the Solar Nebula. (Doctoral Dissertation). University of Colorado. Retrieved from http://scholar.colorado.edu/astr_gradetds/7

Chicago Manual of Style (16th Edition):

Hughes, Anna Louise Haugsjaa. “Mixing of Dust in Protoplanetary Disks and the Solar Nebula.” 2011. Doctoral Dissertation, University of Colorado. Accessed July 20, 2019. http://scholar.colorado.edu/astr_gradetds/7.

MLA Handbook (7th Edition):

Hughes, Anna Louise Haugsjaa. “Mixing of Dust in Protoplanetary Disks and the Solar Nebula.” 2011. Web. 20 Jul 2019.

Vancouver:

Hughes ALH. Mixing of Dust in Protoplanetary Disks and the Solar Nebula. [Internet] [Doctoral dissertation]. University of Colorado; 2011. [cited 2019 Jul 20]. Available from: http://scholar.colorado.edu/astr_gradetds/7.

Council of Science Editors:

Hughes ALH. Mixing of Dust in Protoplanetary Disks and the Solar Nebula. [Doctoral Dissertation]. University of Colorado; 2011. Available from: http://scholar.colorado.edu/astr_gradetds/7


The Ohio State University

16. Fausnaugh, Michael Martin. Reverberation Mapping of the Continuum Source in Active Galactic Nuclei.

Degree: PhD, Astronomy, 2017, The Ohio State University

 I present results from a monitoring campaign of 11 active galacticnuclei (AGN) conducted in Spring of 2014. I use the reverberationmapping method to probe the… (more)

Subjects/Keywords: Astronomy; Astrophysics; Astronomy; Astrophysics; Black Holes; Active Galaxies; Accretion Disks

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APA (6th Edition):

Fausnaugh, M. M. (2017). Reverberation Mapping of the Continuum Source in Active Galactic Nuclei. (Doctoral Dissertation). The Ohio State University. Retrieved from http://rave.ohiolink.edu/etdc/view?acc_num=osu1494244528720735

Chicago Manual of Style (16th Edition):

Fausnaugh, Michael Martin. “Reverberation Mapping of the Continuum Source in Active Galactic Nuclei.” 2017. Doctoral Dissertation, The Ohio State University. Accessed July 20, 2019. http://rave.ohiolink.edu/etdc/view?acc_num=osu1494244528720735.

MLA Handbook (7th Edition):

Fausnaugh, Michael Martin. “Reverberation Mapping of the Continuum Source in Active Galactic Nuclei.” 2017. Web. 20 Jul 2019.

Vancouver:

Fausnaugh MM. Reverberation Mapping of the Continuum Source in Active Galactic Nuclei. [Internet] [Doctoral dissertation]. The Ohio State University; 2017. [cited 2019 Jul 20]. Available from: http://rave.ohiolink.edu/etdc/view?acc_num=osu1494244528720735.

Council of Science Editors:

Fausnaugh MM. Reverberation Mapping of the Continuum Source in Active Galactic Nuclei. [Doctoral Dissertation]. The Ohio State University; 2017. Available from: http://rave.ohiolink.edu/etdc/view?acc_num=osu1494244528720735


Universiteit Utrecht

17. Blokland, J.W.S. Equilibrium and stability of tokamak plasmas and accretion disks.

Degree: 2007, Universiteit Utrecht

 In both fusion research as well in astrophysics, plasmas are widely studied. These plasmas can be found in different geometric configurations, such as in a… (more)

Subjects/Keywords: Natuur- en Sterrenkunde; magnetohydrodynamics; equilibrium; stability; tokamak plasmas; accretion disks

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APA (6th Edition):

Blokland, J. W. S. (2007). Equilibrium and stability of tokamak plasmas and accretion disks. (Doctoral Dissertation). Universiteit Utrecht. Retrieved from http://dspace.library.uu.nl:8080/handle/1874/22651

Chicago Manual of Style (16th Edition):

Blokland, J W S. “Equilibrium and stability of tokamak plasmas and accretion disks.” 2007. Doctoral Dissertation, Universiteit Utrecht. Accessed July 20, 2019. http://dspace.library.uu.nl:8080/handle/1874/22651.

MLA Handbook (7th Edition):

Blokland, J W S. “Equilibrium and stability of tokamak plasmas and accretion disks.” 2007. Web. 20 Jul 2019.

Vancouver:

Blokland JWS. Equilibrium and stability of tokamak plasmas and accretion disks. [Internet] [Doctoral dissertation]. Universiteit Utrecht; 2007. [cited 2019 Jul 20]. Available from: http://dspace.library.uu.nl:8080/handle/1874/22651.

Council of Science Editors:

Blokland JWS. Equilibrium and stability of tokamak plasmas and accretion disks. [Doctoral Dissertation]. Universiteit Utrecht; 2007. Available from: http://dspace.library.uu.nl:8080/handle/1874/22651


Penn State University

18. Lewis, Karen Theresa. Unveiling the Accretion Disks that Fuel Active Galactic Nuclei.

Degree: PhD, Astronomy and Astrophysics, 2005, Penn State University

 An increasing number of Active Galactic Nuclei (AGN) exhibit broad, double-peaked Balmer emission lines, reminiscent of those observed in Cataclysmic Variables; these double-peaked Balmer lines… (more)

Subjects/Keywords: active galactic nuclei; accretion disks

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APA (6th Edition):

Lewis, K. T. (2005). Unveiling the Accretion Disks that Fuel Active Galactic Nuclei. (Doctoral Dissertation). Penn State University. Retrieved from https://etda.libraries.psu.edu/catalog/6771

Chicago Manual of Style (16th Edition):

Lewis, Karen Theresa. “Unveiling the Accretion Disks that Fuel Active Galactic Nuclei.” 2005. Doctoral Dissertation, Penn State University. Accessed July 20, 2019. https://etda.libraries.psu.edu/catalog/6771.

MLA Handbook (7th Edition):

Lewis, Karen Theresa. “Unveiling the Accretion Disks that Fuel Active Galactic Nuclei.” 2005. Web. 20 Jul 2019.

Vancouver:

Lewis KT. Unveiling the Accretion Disks that Fuel Active Galactic Nuclei. [Internet] [Doctoral dissertation]. Penn State University; 2005. [cited 2019 Jul 20]. Available from: https://etda.libraries.psu.edu/catalog/6771.

Council of Science Editors:

Lewis KT. Unveiling the Accretion Disks that Fuel Active Galactic Nuclei. [Doctoral Dissertation]. Penn State University; 2005. Available from: https://etda.libraries.psu.edu/catalog/6771


Louisiana State University

19. Bradley, Charles. Studies of states and state transitions in low mass X-ray binaries.

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

 We investigate the model of a disk/coronal accretion flow into a black hole. We build a numerical code to ascertain whether the inner regions of… (more)

Subjects/Keywords: mass transfer; black holes; accretion disks; binary stars

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APA (6th Edition):

Bradley, C. (2009). Studies of states and state transitions in low mass X-ray binaries. (Doctoral Dissertation). Louisiana State University. Retrieved from etd-07072009-123333 ; https://digitalcommons.lsu.edu/gradschool_dissertations/1708

Chicago Manual of Style (16th Edition):

Bradley, Charles. “Studies of states and state transitions in low mass X-ray binaries.” 2009. Doctoral Dissertation, Louisiana State University. Accessed July 20, 2019. etd-07072009-123333 ; https://digitalcommons.lsu.edu/gradschool_dissertations/1708.

MLA Handbook (7th Edition):

Bradley, Charles. “Studies of states and state transitions in low mass X-ray binaries.” 2009. Web. 20 Jul 2019.

Vancouver:

Bradley C. Studies of states and state transitions in low mass X-ray binaries. [Internet] [Doctoral dissertation]. Louisiana State University; 2009. [cited 2019 Jul 20]. Available from: etd-07072009-123333 ; https://digitalcommons.lsu.edu/gradschool_dissertations/1708.

Council of Science Editors:

Bradley C. Studies of states and state transitions in low mass X-ray binaries. [Doctoral Dissertation]. Louisiana State University; 2009. Available from: etd-07072009-123333 ; https://digitalcommons.lsu.edu/gradschool_dissertations/1708


Clemson University

20. Liskowsky, Joseph. FUor and EXor Variables: A NIR High-Resolution Spectroscopic Survey.

Degree: MS, Physics and Astronomy, 2010, Clemson University

 To better understand the labyrinth of heating and cooling processes in YSOs (young stellar objects), we study systems where there exists a large variability in… (more)

Subjects/Keywords: accretion; disks; FUor; FU Orionis; Astrophysics and Astronomy

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APA (6th Edition):

Liskowsky, J. (2010). FUor and EXor Variables: A NIR High-Resolution Spectroscopic Survey. (Masters Thesis). Clemson University. Retrieved from https://tigerprints.clemson.edu/all_theses/977

Chicago Manual of Style (16th Edition):

Liskowsky, Joseph. “FUor and EXor Variables: A NIR High-Resolution Spectroscopic Survey.” 2010. Masters Thesis, Clemson University. Accessed July 20, 2019. https://tigerprints.clemson.edu/all_theses/977.

MLA Handbook (7th Edition):

Liskowsky, Joseph. “FUor and EXor Variables: A NIR High-Resolution Spectroscopic Survey.” 2010. Web. 20 Jul 2019.

Vancouver:

Liskowsky J. FUor and EXor Variables: A NIR High-Resolution Spectroscopic Survey. [Internet] [Masters thesis]. Clemson University; 2010. [cited 2019 Jul 20]. Available from: https://tigerprints.clemson.edu/all_theses/977.

Council of Science Editors:

Liskowsky J. FUor and EXor Variables: A NIR High-Resolution Spectroscopic Survey. [Masters Thesis]. Clemson University; 2010. Available from: https://tigerprints.clemson.edu/all_theses/977


University of Illinois – Urbana-Champaign

21. Ryan, Benjamin Ransom. General relativistic radiation magnetohydrodynamics, with applications to black hole accretion disks.

Degree: PhD, Astronomy, 2018, University of Illinois – Urbana-Champaign

 Electron temperatures in the inner region of accretion disks around black holes are set by the balance of advection, viscous heating, and radiative interactions. At… (more)

Subjects/Keywords: Black holes; Accretion disks; radiation hydrodynamics; magnetohydrodynamics; Monte Carlo methods; M87

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APA (6th Edition):

Ryan, B. R. (2018). General relativistic radiation magnetohydrodynamics, with applications to black hole accretion disks. (Doctoral Dissertation). University of Illinois – Urbana-Champaign. Retrieved from http://hdl.handle.net/2142/101012

Chicago Manual of Style (16th Edition):

Ryan, Benjamin Ransom. “General relativistic radiation magnetohydrodynamics, with applications to black hole accretion disks.” 2018. Doctoral Dissertation, University of Illinois – Urbana-Champaign. Accessed July 20, 2019. http://hdl.handle.net/2142/101012.

MLA Handbook (7th Edition):

Ryan, Benjamin Ransom. “General relativistic radiation magnetohydrodynamics, with applications to black hole accretion disks.” 2018. Web. 20 Jul 2019.

Vancouver:

Ryan BR. General relativistic radiation magnetohydrodynamics, with applications to black hole accretion disks. [Internet] [Doctoral dissertation]. University of Illinois – Urbana-Champaign; 2018. [cited 2019 Jul 20]. Available from: http://hdl.handle.net/2142/101012.

Council of Science Editors:

Ryan BR. General relativistic radiation magnetohydrodynamics, with applications to black hole accretion disks. [Doctoral Dissertation]. University of Illinois – Urbana-Champaign; 2018. Available from: http://hdl.handle.net/2142/101012


Rochester Institute of Technology

22. Principe, David A. Multiwavelength Observations of Young Stars and Their Circumstellar Disks.

Degree: PhD, School of Physics and Astronomy (COS), 2014, Rochester Institute of Technology

  Observational studies of star and planet formation represent a fundamental means to understand the origins of exoplanetary systems and our own solar system. In… (more)

Subjects/Keywords: Accretion; Circumstellar disks; Magnetic fields; Pre-MS stars; Star formation

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APA (6th Edition):

Principe, D. A. (2014). Multiwavelength Observations of Young Stars and Their Circumstellar Disks. (Doctoral Dissertation). Rochester Institute of Technology. Retrieved from https://scholarworks.rit.edu/theses/8371

Chicago Manual of Style (16th Edition):

Principe, David A. “Multiwavelength Observations of Young Stars and Their Circumstellar Disks.” 2014. Doctoral Dissertation, Rochester Institute of Technology. Accessed July 20, 2019. https://scholarworks.rit.edu/theses/8371.

MLA Handbook (7th Edition):

Principe, David A. “Multiwavelength Observations of Young Stars and Their Circumstellar Disks.” 2014. Web. 20 Jul 2019.

Vancouver:

Principe DA. Multiwavelength Observations of Young Stars and Their Circumstellar Disks. [Internet] [Doctoral dissertation]. Rochester Institute of Technology; 2014. [cited 2019 Jul 20]. Available from: https://scholarworks.rit.edu/theses/8371.

Council of Science Editors:

Principe DA. Multiwavelength Observations of Young Stars and Their Circumstellar Disks. [Doctoral Dissertation]. Rochester Institute of Technology; 2014. Available from: https://scholarworks.rit.edu/theses/8371

23. Thomson, Brent. Determining The Origin And Possible Mechanisms Of QPOS In X-Ray Emissions Of Neutron Stars And Black Holes.

Degree: PhD, Physics & Astrophysics, 2014, University of North Dakota

  QPOs (Quasi-Periodic Oscillations) are time oscillations that appear in the light curve of observational data in x-ray bands. They are of mysterious origin although… (more)

Subjects/Keywords: accretion disks; astrophysics; compact objects; quasi-periodic oscillations; x-ray radiation

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APA (6th Edition):

Thomson, B. (2014). Determining The Origin And Possible Mechanisms Of QPOS In X-Ray Emissions Of Neutron Stars And Black Holes. (Doctoral Dissertation). University of North Dakota. Retrieved from https://commons.und.edu/theses/1721

Chicago Manual of Style (16th Edition):

Thomson, Brent. “Determining The Origin And Possible Mechanisms Of QPOS In X-Ray Emissions Of Neutron Stars And Black Holes.” 2014. Doctoral Dissertation, University of North Dakota. Accessed July 20, 2019. https://commons.und.edu/theses/1721.

MLA Handbook (7th Edition):

Thomson, Brent. “Determining The Origin And Possible Mechanisms Of QPOS In X-Ray Emissions Of Neutron Stars And Black Holes.” 2014. Web. 20 Jul 2019.

Vancouver:

Thomson B. Determining The Origin And Possible Mechanisms Of QPOS In X-Ray Emissions Of Neutron Stars And Black Holes. [Internet] [Doctoral dissertation]. University of North Dakota; 2014. [cited 2019 Jul 20]. Available from: https://commons.und.edu/theses/1721.

Council of Science Editors:

Thomson B. Determining The Origin And Possible Mechanisms Of QPOS In X-Ray Emissions Of Neutron Stars And Black Holes. [Doctoral Dissertation]. University of North Dakota; 2014. Available from: https://commons.und.edu/theses/1721


Ohio University

24. Finke, Justin David. Monte Carlo/Fokker-Planck simulations of Accretion Phenomena and Optical Spectra of BL Lacertae Objects.

Degree: PhD, Physics (Arts and Sciences), 2007, Ohio University

  A time-dependent two-dimensional Monte Carlo/Fokker-Planck (MC/FP) code, which uses a Monte Carlo technique for Compton scattering and radiative transport, and a Fokker-Planck technique for… (more)

Subjects/Keywords: Physics, Astronomy and Astrophysics; X-rays: binaries; radiative transfer; methods: numerical; BL Lacertae objects; accretion, accretion disks

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APA (6th Edition):

Finke, J. D. (2007). Monte Carlo/Fokker-Planck simulations of Accretion Phenomena and Optical Spectra of BL Lacertae Objects. (Doctoral Dissertation). Ohio University. Retrieved from http://rave.ohiolink.edu/etdc/view?acc_num=ohiou1181833339

Chicago Manual of Style (16th Edition):

Finke, Justin David. “Monte Carlo/Fokker-Planck simulations of Accretion Phenomena and Optical Spectra of BL Lacertae Objects.” 2007. Doctoral Dissertation, Ohio University. Accessed July 20, 2019. http://rave.ohiolink.edu/etdc/view?acc_num=ohiou1181833339.

MLA Handbook (7th Edition):

Finke, Justin David. “Monte Carlo/Fokker-Planck simulations of Accretion Phenomena and Optical Spectra of BL Lacertae Objects.” 2007. Web. 20 Jul 2019.

Vancouver:

Finke JD. Monte Carlo/Fokker-Planck simulations of Accretion Phenomena and Optical Spectra of BL Lacertae Objects. [Internet] [Doctoral dissertation]. Ohio University; 2007. [cited 2019 Jul 20]. Available from: http://rave.ohiolink.edu/etdc/view?acc_num=ohiou1181833339.

Council of Science Editors:

Finke JD. Monte Carlo/Fokker-Planck simulations of Accretion Phenomena and Optical Spectra of BL Lacertae Objects. [Doctoral Dissertation]. Ohio University; 2007. Available from: http://rave.ohiolink.edu/etdc/view?acc_num=ohiou1181833339


Universitat de Valencia

25. Vives Arias, Héctor. Gravitational Lensing: the Structure of Quasars and Galaxies .

Degree: 2016, Universitat de Valencia

 We use gravitational lens systems in which a galaxy produces multiple images of a distant quasar to study the properties of both the unresolved structure… (more)

Subjects/Keywords: Q2237+0305; gravitational lensing; dark matter; Einstein Cross; microlensing; galaxies; mid-infrared; radio; accretion; accretion disks; quasars; strong lensing

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APA (6th Edition):

Vives Arias, H. (2016). Gravitational Lensing: the Structure of Quasars and Galaxies . (Doctoral Dissertation). Universitat de Valencia. Retrieved from http://hdl.handle.net/10550/56465

Chicago Manual of Style (16th Edition):

Vives Arias, Héctor. “Gravitational Lensing: the Structure of Quasars and Galaxies .” 2016. Doctoral Dissertation, Universitat de Valencia. Accessed July 20, 2019. http://hdl.handle.net/10550/56465.

MLA Handbook (7th Edition):

Vives Arias, Héctor. “Gravitational Lensing: the Structure of Quasars and Galaxies .” 2016. Web. 20 Jul 2019.

Vancouver:

Vives Arias H. Gravitational Lensing: the Structure of Quasars and Galaxies . [Internet] [Doctoral dissertation]. Universitat de Valencia; 2016. [cited 2019 Jul 20]. Available from: http://hdl.handle.net/10550/56465.

Council of Science Editors:

Vives Arias H. Gravitational Lensing: the Structure of Quasars and Galaxies . [Doctoral Dissertation]. Universitat de Valencia; 2016. Available from: http://hdl.handle.net/10550/56465

26. Flaherty, Kevin. Young stellar objects in lynds 1641: Disks, accretion, and star formation history.

Degree: 2018, The American Astronomical Society

Subjects/Keywords: Accretion, accretion disks; Protoplanetary disks; Stars: pre-main sequence; Física

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APA (6th Edition):

Flaherty, K. (2018). Young stellar objects in lynds 1641: Disks, accretion, and star formation history. (Thesis). The American Astronomical Society. Retrieved from http://hdl.handle.net/10486/662090

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):

Flaherty, Kevin. “Young stellar objects in lynds 1641: Disks, accretion, and star formation history.” 2018. Thesis, The American Astronomical Society. Accessed July 20, 2019. http://hdl.handle.net/10486/662090.

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

MLA Handbook (7th Edition):

Flaherty, Kevin. “Young stellar objects in lynds 1641: Disks, accretion, and star formation history.” 2018. Web. 20 Jul 2019.

Vancouver:

Flaherty K. Young stellar objects in lynds 1641: Disks, accretion, and star formation history. [Internet] [Thesis]. The American Astronomical Society; 2018. [cited 2019 Jul 20]. Available from: http://hdl.handle.net/10486/662090.

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

Council of Science Editors:

Flaherty K. Young stellar objects in lynds 1641: Disks, accretion, and star formation history. [Thesis]. The American Astronomical Society; 2018. Available from: http://hdl.handle.net/10486/662090

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


Rochester Institute of Technology

27. Gupte, Tanmayee. Smoothed Particle Hydrodynamics.

Degree: MS, School of Physics and Astronomy (COS), 2018, Rochester Institute of Technology

  Smoothed particle hydrodynamics (SPH) is a meshfree particle method based on a Lagrangian formulation, which has been widely applied to different areas in astrophysics… (more)

Subjects/Keywords: Accretion disks; Astrophysics; Computational fluid dynamics; Neutron stars; Shock tube test; Smoothed particle hydrodynamics

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APA (6th Edition):

Gupte, T. (2018). Smoothed Particle Hydrodynamics. (Masters Thesis). Rochester Institute of Technology. Retrieved from https://scholarworks.rit.edu/theses/9848

Chicago Manual of Style (16th Edition):

Gupte, Tanmayee. “Smoothed Particle Hydrodynamics.” 2018. Masters Thesis, Rochester Institute of Technology. Accessed July 20, 2019. https://scholarworks.rit.edu/theses/9848.

MLA Handbook (7th Edition):

Gupte, Tanmayee. “Smoothed Particle Hydrodynamics.” 2018. Web. 20 Jul 2019.

Vancouver:

Gupte T. Smoothed Particle Hydrodynamics. [Internet] [Masters thesis]. Rochester Institute of Technology; 2018. [cited 2019 Jul 20]. Available from: https://scholarworks.rit.edu/theses/9848.

Council of Science Editors:

Gupte T. Smoothed Particle Hydrodynamics. [Masters Thesis]. Rochester Institute of Technology; 2018. Available from: https://scholarworks.rit.edu/theses/9848


University College Cork

28. O'Riordan, Michael. Radiative signatures of the jet launching region in astronomical objects.

Degree: 2018, University College Cork

 Relativistic jets are observed in a wide range of accreting black hole systems, from stellar-mass black holes in X-ray binaries (XRBs), to supermassive black holes… (more)

Subjects/Keywords: Black hole physics; Jets; Radiative processes; High-energy astrophysics; Accretion disks; Relativistic processes

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APA (6th Edition):

O'Riordan, M. (2018). Radiative signatures of the jet launching region in astronomical objects. (Thesis). University College Cork. Retrieved from http://hdl.handle.net/10468/6124

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):

O'Riordan, Michael. “Radiative signatures of the jet launching region in astronomical objects.” 2018. Thesis, University College Cork. Accessed July 20, 2019. http://hdl.handle.net/10468/6124.

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

MLA Handbook (7th Edition):

O'Riordan, Michael. “Radiative signatures of the jet launching region in astronomical objects.” 2018. Web. 20 Jul 2019.

Vancouver:

O'Riordan M. Radiative signatures of the jet launching region in astronomical objects. [Internet] [Thesis]. University College Cork; 2018. [cited 2019 Jul 20]. Available from: http://hdl.handle.net/10468/6124.

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

Council of Science Editors:

O'Riordan M. Radiative signatures of the jet launching region in astronomical objects. [Thesis]. University College Cork; 2018. Available from: http://hdl.handle.net/10468/6124

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


Washington State University

29. [No author]. Neutrinos in Mergers of Neutron Stars with Black Holes .

Degree: 2015, Washington State University

 Mergers of a neutron star and a black hole are interesting because of the dual complexity of the black hole's strong gravity and the neutron… (more)

Subjects/Keywords: Astrophysics; Physics; Astronomy; Black Holes; Compact Object Mergers; Neutrinos; Neutron Stars; Nuclear Accretion Disks

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APA (6th Edition):

author], [. (2015). Neutrinos in Mergers of Neutron Stars with Black Holes . (Thesis). Washington State University. Retrieved from http://hdl.handle.net/2376/6157

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):

author], [No. “Neutrinos in Mergers of Neutron Stars with Black Holes .” 2015. Thesis, Washington State University. Accessed July 20, 2019. http://hdl.handle.net/2376/6157.

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

MLA Handbook (7th Edition):

author], [No. “Neutrinos in Mergers of Neutron Stars with Black Holes .” 2015. Web. 20 Jul 2019.

Vancouver:

author] [. Neutrinos in Mergers of Neutron Stars with Black Holes . [Internet] [Thesis]. Washington State University; 2015. [cited 2019 Jul 20]. Available from: http://hdl.handle.net/2376/6157.

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

Council of Science Editors:

author] [. Neutrinos in Mergers of Neutron Stars with Black Holes . [Thesis]. Washington State University; 2015. Available from: http://hdl.handle.net/2376/6157

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

30. Coleman, Matthew Singh Bawa. Convection Affects Magnetic Turbulence in White Dwarf Accretion Disks.

Degree: 2017, University of California – eScholarship, University of California

 In this dissertation we focus on the accretion disks which surround accreting white dwarfs as they are some of the most abundant and well observed… (more)

Subjects/Keywords: Astrophysics; accretion disks; cataclysmic variables; convection; dwarf novae; MHD turbulence; white dwarfs

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APA (6th Edition):

Coleman, M. S. B. (2017). Convection Affects Magnetic Turbulence in White Dwarf Accretion Disks. (Thesis). University of California – eScholarship, University of California. Retrieved from http://www.escholarship.org/uc/item/5fk2m1jv

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):

Coleman, Matthew Singh Bawa. “Convection Affects Magnetic Turbulence in White Dwarf Accretion Disks.” 2017. Thesis, University of California – eScholarship, University of California. Accessed July 20, 2019. http://www.escholarship.org/uc/item/5fk2m1jv.

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

MLA Handbook (7th Edition):

Coleman, Matthew Singh Bawa. “Convection Affects Magnetic Turbulence in White Dwarf Accretion Disks.” 2017. Web. 20 Jul 2019.

Vancouver:

Coleman MSB. Convection Affects Magnetic Turbulence in White Dwarf Accretion Disks. [Internet] [Thesis]. University of California – eScholarship, University of California; 2017. [cited 2019 Jul 20]. Available from: http://www.escholarship.org/uc/item/5fk2m1jv.

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

Council of Science Editors:

Coleman MSB. Convection Affects Magnetic Turbulence in White Dwarf Accretion Disks. [Thesis]. University of California – eScholarship, University of California; 2017. Available from: http://www.escholarship.org/uc/item/5fk2m1jv

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

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