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You searched for subject:(Stellar dynamics). Showing records 1 – 30 of 39 total matches.

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University of Maryland

1. Gill, Michael Allen. The Dynamics of Dense Stellar Systems with a Massive Black Hole.

Degree: Astronomy, 2011, University of Maryland

 In this work, we explore the dynamics of two similar types of dense stellar systems with a central black hole of mass much greater than… (more)

Subjects/Keywords: Astrophysics; black holes; stellar dynamics

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APA (6th Edition):

Gill, M. A. (2011). The Dynamics of Dense Stellar Systems with a Massive Black Hole. (Thesis). University of Maryland. Retrieved from http://hdl.handle.net/1903/11986

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):

Gill, Michael Allen. “The Dynamics of Dense Stellar Systems with a Massive Black Hole.” 2011. Thesis, University of Maryland. Accessed October 20, 2020. http://hdl.handle.net/1903/11986.

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

MLA Handbook (7th Edition):

Gill, Michael Allen. “The Dynamics of Dense Stellar Systems with a Massive Black Hole.” 2011. Web. 20 Oct 2020.

Vancouver:

Gill MA. The Dynamics of Dense Stellar Systems with a Massive Black Hole. [Internet] [Thesis]. University of Maryland; 2011. [cited 2020 Oct 20]. Available from: http://hdl.handle.net/1903/11986.

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

Council of Science Editors:

Gill MA. The Dynamics of Dense Stellar Systems with a Massive Black Hole. [Thesis]. University of Maryland; 2011. Available from: http://hdl.handle.net/1903/11986

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


Columbia University

2. Generozov, Aleksey. Stellar and gas dynamics in galactic nuclei.

Degree: 2018, Columbia University

 Galactic nuclei are important for studies of galaxy evolution, stellar dynamics and general relativity. Many have Supermassive Black Holes (SMBHs) (with one million to one… (more)

Subjects/Keywords: Astronomy; Stellar dynamics; Gas dynamics; Galactic nuclei

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APA (6th Edition):

Generozov, A. (2018). Stellar and gas dynamics in galactic nuclei. (Doctoral Dissertation). Columbia University. Retrieved from https://doi.org/10.7916/D8087NVH

Chicago Manual of Style (16th Edition):

Generozov, Aleksey. “Stellar and gas dynamics in galactic nuclei.” 2018. Doctoral Dissertation, Columbia University. Accessed October 20, 2020. https://doi.org/10.7916/D8087NVH.

MLA Handbook (7th Edition):

Generozov, Aleksey. “Stellar and gas dynamics in galactic nuclei.” 2018. Web. 20 Oct 2020.

Vancouver:

Generozov A. Stellar and gas dynamics in galactic nuclei. [Internet] [Doctoral dissertation]. Columbia University; 2018. [cited 2020 Oct 20]. Available from: https://doi.org/10.7916/D8087NVH.

Council of Science Editors:

Generozov A. Stellar and gas dynamics in galactic nuclei. [Doctoral Dissertation]. Columbia University; 2018. Available from: https://doi.org/10.7916/D8087NVH

3. Silva, Manuel Duarte de Vasconcelos. Runaway stars in the Galactic halo : their origin and kinematics.

Degree: PhD, 2012, University of Hertfordshire

 Star formation in the Milky Way is confined to star-forming regions (OB association, HII regions, and open clusters) in the Galactic plane. It is usually… (more)

Subjects/Keywords: 520; Runaway stars; Early-type stars; stellar kinematics; stellar dynamics; Milky Way; spiral arms

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APA (6th Edition):

Silva, M. D. d. V. (2012). Runaway stars in the Galactic halo : their origin and kinematics. (Doctoral Dissertation). University of Hertfordshire. Retrieved from http://hdl.handle.net/2299/8115

Chicago Manual of Style (16th Edition):

Silva, Manuel Duarte de Vasconcelos. “Runaway stars in the Galactic halo : their origin and kinematics.” 2012. Doctoral Dissertation, University of Hertfordshire. Accessed October 20, 2020. http://hdl.handle.net/2299/8115.

MLA Handbook (7th Edition):

Silva, Manuel Duarte de Vasconcelos. “Runaway stars in the Galactic halo : their origin and kinematics.” 2012. Web. 20 Oct 2020.

Vancouver:

Silva MDdV. Runaway stars in the Galactic halo : their origin and kinematics. [Internet] [Doctoral dissertation]. University of Hertfordshire; 2012. [cited 2020 Oct 20]. Available from: http://hdl.handle.net/2299/8115.

Council of Science Editors:

Silva MDdV. Runaway stars in the Galactic halo : their origin and kinematics. [Doctoral Dissertation]. University of Hertfordshire; 2012. Available from: http://hdl.handle.net/2299/8115


UCLA

4. Frewen, Shane Franklin Nishi. Eccentric Planets around Evolved Stars.

Degree: Astronomy, 2015, UCLA

 Planets are now known to be near ubiquitous around main-sequence stars in our galaxy, as evidenced by the results of radial velocity and transit surveys… (more)

Subjects/Keywords: Astrophysics; Astronomy; Dynamics; Extrasolar planets; Stellar evolution; Warm jupiters; White dwarfs

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APA (6th Edition):

Frewen, S. F. N. (2015). Eccentric Planets around Evolved Stars. (Thesis). UCLA. Retrieved from http://www.escholarship.org/uc/item/7qx5n8fd

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):

Frewen, Shane Franklin Nishi. “Eccentric Planets around Evolved Stars.” 2015. Thesis, UCLA. Accessed October 20, 2020. http://www.escholarship.org/uc/item/7qx5n8fd.

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

MLA Handbook (7th Edition):

Frewen, Shane Franklin Nishi. “Eccentric Planets around Evolved Stars.” 2015. Web. 20 Oct 2020.

Vancouver:

Frewen SFN. Eccentric Planets around Evolved Stars. [Internet] [Thesis]. UCLA; 2015. [cited 2020 Oct 20]. Available from: http://www.escholarship.org/uc/item/7qx5n8fd.

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

Council of Science Editors:

Frewen SFN. Eccentric Planets around Evolved Stars. [Thesis]. UCLA; 2015. Available from: http://www.escholarship.org/uc/item/7qx5n8fd

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


University of California – Berkeley

5. Converse, Joseph Mitchell. The Initial Conditions and Evolution of Open Clusters.

Degree: Astrophysics, 2010, University of California – Berkeley

 Despite being some of the most familiar objects observed in the sky, much remains unknown about open clusters. The theory of their formation admits many… (more)

Subjects/Keywords: Astrophysics; Alpha Persei; Pleiades; Star Clusters; Stellar Dynamics

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APA (6th Edition):

Converse, J. M. (2010). The Initial Conditions and Evolution of Open Clusters. (Thesis). University of California – Berkeley. Retrieved from http://www.escholarship.org/uc/item/48f1d45h

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):

Converse, Joseph Mitchell. “The Initial Conditions and Evolution of Open Clusters.” 2010. Thesis, University of California – Berkeley. Accessed October 20, 2020. http://www.escholarship.org/uc/item/48f1d45h.

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

MLA Handbook (7th Edition):

Converse, Joseph Mitchell. “The Initial Conditions and Evolution of Open Clusters.” 2010. Web. 20 Oct 2020.

Vancouver:

Converse JM. The Initial Conditions and Evolution of Open Clusters. [Internet] [Thesis]. University of California – Berkeley; 2010. [cited 2020 Oct 20]. Available from: http://www.escholarship.org/uc/item/48f1d45h.

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

Council of Science Editors:

Converse JM. The Initial Conditions and Evolution of Open Clusters. [Thesis]. University of California – Berkeley; 2010. Available from: http://www.escholarship.org/uc/item/48f1d45h

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


University of Michigan

6. Kounkel, Marina. Distances, Kinematics, and Structure of Nearby Star-Forming Regions.

Degree: PhD, Astronomy and Astrophysics, 2017, University of Michigan

 In this thesis I present an analysis of the structure and kinematics of the Orion Molecular Cloud Complex in an effort to better characterize the… (more)

Subjects/Keywords: stellar kinematics and dynamics; young star clusters; Astronomy; Science

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APA (6th Edition):

Kounkel, M. (2017). Distances, Kinematics, and Structure of Nearby Star-Forming Regions. (Doctoral Dissertation). University of Michigan. Retrieved from http://hdl.handle.net/2027.42/140833

Chicago Manual of Style (16th Edition):

Kounkel, Marina. “Distances, Kinematics, and Structure of Nearby Star-Forming Regions.” 2017. Doctoral Dissertation, University of Michigan. Accessed October 20, 2020. http://hdl.handle.net/2027.42/140833.

MLA Handbook (7th Edition):

Kounkel, Marina. “Distances, Kinematics, and Structure of Nearby Star-Forming Regions.” 2017. Web. 20 Oct 2020.

Vancouver:

Kounkel M. Distances, Kinematics, and Structure of Nearby Star-Forming Regions. [Internet] [Doctoral dissertation]. University of Michigan; 2017. [cited 2020 Oct 20]. Available from: http://hdl.handle.net/2027.42/140833.

Council of Science Editors:

Kounkel M. Distances, Kinematics, and Structure of Nearby Star-Forming Regions. [Doctoral Dissertation]. University of Michigan; 2017. Available from: http://hdl.handle.net/2027.42/140833


Durham University

7. Gledhill, Timothy Michael. Optical polarimetry of star forming regions.

Degree: PhD, 1987, Durham University

Subjects/Keywords: 523.01; Stellar evolution dynamics

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APA (6th Edition):

Gledhill, T. M. (1987). Optical polarimetry of star forming regions. (Doctoral Dissertation). Durham University. Retrieved from http://etheses.dur.ac.uk/6757/ ; http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.379703

Chicago Manual of Style (16th Edition):

Gledhill, Timothy Michael. “Optical polarimetry of star forming regions.” 1987. Doctoral Dissertation, Durham University. Accessed October 20, 2020. http://etheses.dur.ac.uk/6757/ ; http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.379703.

MLA Handbook (7th Edition):

Gledhill, Timothy Michael. “Optical polarimetry of star forming regions.” 1987. Web. 20 Oct 2020.

Vancouver:

Gledhill TM. Optical polarimetry of star forming regions. [Internet] [Doctoral dissertation]. Durham University; 1987. [cited 2020 Oct 20]. Available from: http://etheses.dur.ac.uk/6757/ ; http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.379703.

Council of Science Editors:

Gledhill TM. Optical polarimetry of star forming regions. [Doctoral Dissertation]. Durham University; 1987. Available from: http://etheses.dur.ac.uk/6757/ ; http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.379703


University of Cambridge

8. Loi, Shyeh Tjing. Magnetic fields and stellar oscillations.

Degree: PhD, 2019, University of Cambridge

 Stars are fluid bodies in which pressure, buoyancy, rotation and magnetism provide the restoring forces for wave propagation. Constructive interference of these waves generates global… (more)

Subjects/Keywords: astrophysics; fluid dynamics; magnetohydrodynamics; stars; magnetic fields; stellar oscillations; asteroseismology; gravity waves; internal waves; stellar interiors

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APA (6th Edition):

Loi, S. T. (2019). Magnetic fields and stellar oscillations. (Doctoral Dissertation). University of Cambridge. Retrieved from https://doi.org/10.17863/CAM.40407 ; https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.782768

Chicago Manual of Style (16th Edition):

Loi, Shyeh Tjing. “Magnetic fields and stellar oscillations.” 2019. Doctoral Dissertation, University of Cambridge. Accessed October 20, 2020. https://doi.org/10.17863/CAM.40407 ; https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.782768.

MLA Handbook (7th Edition):

Loi, Shyeh Tjing. “Magnetic fields and stellar oscillations.” 2019. Web. 20 Oct 2020.

Vancouver:

Loi ST. Magnetic fields and stellar oscillations. [Internet] [Doctoral dissertation]. University of Cambridge; 2019. [cited 2020 Oct 20]. Available from: https://doi.org/10.17863/CAM.40407 ; https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.782768.

Council of Science Editors:

Loi ST. Magnetic fields and stellar oscillations. [Doctoral Dissertation]. University of Cambridge; 2019. Available from: https://doi.org/10.17863/CAM.40407 ; https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.782768


University of Cambridge

9. Loi, Shyeh Tjing. Magnetic fields and stellar oscillations.

Degree: PhD, 2019, University of Cambridge

 Stars are fluid bodies in which pressure, buoyancy, rotation and magnetism provide the restoring forces for wave propagation. Constructive interference of these waves generates global… (more)

Subjects/Keywords: astrophysics; fluid dynamics; magnetohydrodynamics; stars; magnetic fields; stellar oscillations; asteroseismology; gravity waves; internal waves; stellar interiors

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APA (6th Edition):

Loi, S. T. (2019). Magnetic fields and stellar oscillations. (Doctoral Dissertation). University of Cambridge. Retrieved from https://www.repository.cam.ac.uk/handle/1810/293256

Chicago Manual of Style (16th Edition):

Loi, Shyeh Tjing. “Magnetic fields and stellar oscillations.” 2019. Doctoral Dissertation, University of Cambridge. Accessed October 20, 2020. https://www.repository.cam.ac.uk/handle/1810/293256.

MLA Handbook (7th Edition):

Loi, Shyeh Tjing. “Magnetic fields and stellar oscillations.” 2019. Web. 20 Oct 2020.

Vancouver:

Loi ST. Magnetic fields and stellar oscillations. [Internet] [Doctoral dissertation]. University of Cambridge; 2019. [cited 2020 Oct 20]. Available from: https://www.repository.cam.ac.uk/handle/1810/293256.

Council of Science Editors:

Loi ST. Magnetic fields and stellar oscillations. [Doctoral Dissertation]. University of Cambridge; 2019. Available from: https://www.repository.cam.ac.uk/handle/1810/293256


University of Colorado

10. Augustson, Kyle C. Convection and Dynamo Action in Massive Stars.

Degree: PhD, Astrophysical & Planetary Sciences, 2013, University of Colorado

  Contact between numerical simulations and observations of stellar magnetism is sought, with an emphasis on those stars that are the most readily observed and… (more)

Subjects/Keywords: Dynamo Theory; Fluid Dynamics; Stellar Convection; Stellar Magnetism; Astrophysics and Astronomy; Physical Processes; Stars, Interstellar Medium and the Galaxy

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APA (6th Edition):

Augustson, K. C. (2013). Convection and Dynamo Action in Massive Stars. (Doctoral Dissertation). University of Colorado. Retrieved from https://scholar.colorado.edu/astr_gradetds/26

Chicago Manual of Style (16th Edition):

Augustson, Kyle C. “Convection and Dynamo Action in Massive Stars.” 2013. Doctoral Dissertation, University of Colorado. Accessed October 20, 2020. https://scholar.colorado.edu/astr_gradetds/26.

MLA Handbook (7th Edition):

Augustson, Kyle C. “Convection and Dynamo Action in Massive Stars.” 2013. Web. 20 Oct 2020.

Vancouver:

Augustson KC. Convection and Dynamo Action in Massive Stars. [Internet] [Doctoral dissertation]. University of Colorado; 2013. [cited 2020 Oct 20]. Available from: https://scholar.colorado.edu/astr_gradetds/26.

Council of Science Editors:

Augustson KC. Convection and Dynamo Action in Massive Stars. [Doctoral Dissertation]. University of Colorado; 2013. Available from: https://scholar.colorado.edu/astr_gradetds/26


Macquarie University

11. Iaconi, Roberto. The impact of initial conditions on simulations of the common envelope binary interaction.

Degree: 2016, Macquarie University

Empirical thesis.

Bibliography: pages 139-144.

1. Introduction  – 2. Our "codes" and the generation of the initial stellar model  – 3. The effect of the… (more)

Subjects/Keywords: Stellar associations  – Mathematical models; Stellar dynamics  – Mathematical models; stars; AGB and post-AGB; evolution; binaries; close; hydrodynamics; methods; numerical

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APA (6th Edition):

Iaconi, R. (2016). The impact of initial conditions on simulations of the common envelope binary interaction. (Doctoral Dissertation). Macquarie University. Retrieved from http://hdl.handle.net/1959.14/1252603

Chicago Manual of Style (16th Edition):

Iaconi, Roberto. “The impact of initial conditions on simulations of the common envelope binary interaction.” 2016. Doctoral Dissertation, Macquarie University. Accessed October 20, 2020. http://hdl.handle.net/1959.14/1252603.

MLA Handbook (7th Edition):

Iaconi, Roberto. “The impact of initial conditions on simulations of the common envelope binary interaction.” 2016. Web. 20 Oct 2020.

Vancouver:

Iaconi R. The impact of initial conditions on simulations of the common envelope binary interaction. [Internet] [Doctoral dissertation]. Macquarie University; 2016. [cited 2020 Oct 20]. Available from: http://hdl.handle.net/1959.14/1252603.

Council of Science Editors:

Iaconi R. The impact of initial conditions on simulations of the common envelope binary interaction. [Doctoral Dissertation]. Macquarie University; 2016. Available from: http://hdl.handle.net/1959.14/1252603


University of Oxford

12. Fermani, Francesco. Modelling the Milky Way stellar halo.

Degree: PhD, 2013, University of Oxford

 We motivate the importance of understanding the kinematics and dynamics of the Milky Way stellar halo both in unravelling the formation history and evolution of… (more)

Subjects/Keywords: 523.1; Astrophysics (theoretical); Milky Way: stellar halo; stars: kinematics and dynamics; stars: Horizontal Branch

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APA (6th Edition):

Fermani, F. (2013). Modelling the Milky Way stellar halo. (Doctoral Dissertation). University of Oxford. Retrieved from http://ora.ox.ac.uk/objects/uuid:bcd70530-506d-46c2-8c99-7f5b8f08f915 ; https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.595989

Chicago Manual of Style (16th Edition):

Fermani, Francesco. “Modelling the Milky Way stellar halo.” 2013. Doctoral Dissertation, University of Oxford. Accessed October 20, 2020. http://ora.ox.ac.uk/objects/uuid:bcd70530-506d-46c2-8c99-7f5b8f08f915 ; https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.595989.

MLA Handbook (7th Edition):

Fermani, Francesco. “Modelling the Milky Way stellar halo.” 2013. Web. 20 Oct 2020.

Vancouver:

Fermani F. Modelling the Milky Way stellar halo. [Internet] [Doctoral dissertation]. University of Oxford; 2013. [cited 2020 Oct 20]. Available from: http://ora.ox.ac.uk/objects/uuid:bcd70530-506d-46c2-8c99-7f5b8f08f915 ; https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.595989.

Council of Science Editors:

Fermani F. Modelling the Milky Way stellar halo. [Doctoral Dissertation]. University of Oxford; 2013. Available from: http://ora.ox.ac.uk/objects/uuid:bcd70530-506d-46c2-8c99-7f5b8f08f915 ; https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.595989


University of Sydney

13. Khanna, Shourya. The GALAH and GAIA surveys: the response of the Galactic disk to non-equilibrium features .

Degree: University of Sydney

 The dynamical history of the Milky Way is complicated. We see a lot of substructure (that is likely accreted), both in spatial density, and in… (more)

Subjects/Keywords: GAIA; GALAH; Galactic Dynamics; Stellar Kinematics

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APA (6th Edition):

Khanna, S. (n.d.). The GALAH and GAIA surveys: the response of the Galactic disk to non-equilibrium features . (Thesis). University of Sydney. Retrieved from http://hdl.handle.net/2123/21641

Note: this citation may be lacking information needed for this citation format:
No year of publication.
Not specified: Masters Thesis or Doctoral Dissertation

Chicago Manual of Style (16th Edition):

Khanna, Shourya. “The GALAH and GAIA surveys: the response of the Galactic disk to non-equilibrium features .” Thesis, University of Sydney. Accessed October 20, 2020. http://hdl.handle.net/2123/21641.

Note: this citation may be lacking information needed for this citation format:
No year of publication.
Not specified: Masters Thesis or Doctoral Dissertation

MLA Handbook (7th Edition):

Khanna, Shourya. “The GALAH and GAIA surveys: the response of the Galactic disk to non-equilibrium features .” Web. 20 Oct 2020.

Note: this citation may be lacking information needed for this citation format:
No year of publication.

Vancouver:

Khanna S. The GALAH and GAIA surveys: the response of the Galactic disk to non-equilibrium features . [Internet] [Thesis]. University of Sydney; [cited 2020 Oct 20]. Available from: http://hdl.handle.net/2123/21641.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation
No year of publication.

Council of Science Editors:

Khanna S. The GALAH and GAIA surveys: the response of the Galactic disk to non-equilibrium features . [Thesis]. University of Sydney; Available from: http://hdl.handle.net/2123/21641

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation
No year of publication.


University of Cambridge

14. Winter, Andrew. The influence of stellar birth environment on protoplanetary disc dispersal.

Degree: PhD, 2019, University of Cambridge

 Protoplanetary discs (PPDs) are the progenitors of planets and represent the material available for their formation. Recent surveys indicate that exoplanetary architectures are diverse and… (more)

Subjects/Keywords: Astronomy; Protoplanetary discs; Star formation; Planet formation; Stellar clusters; Exoplanets; accretion; accretion discs; circumstellar matter; Cygnus OB2; photoevaporation; tidal encounters; stellar dynamics; young stars

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APA (6th Edition):

Winter, A. (2019). The influence of stellar birth environment on protoplanetary disc dispersal. (Doctoral Dissertation). University of Cambridge. Retrieved from https://www.repository.cam.ac.uk/handle/1810/293436

Chicago Manual of Style (16th Edition):

Winter, Andrew. “The influence of stellar birth environment on protoplanetary disc dispersal.” 2019. Doctoral Dissertation, University of Cambridge. Accessed October 20, 2020. https://www.repository.cam.ac.uk/handle/1810/293436.

MLA Handbook (7th Edition):

Winter, Andrew. “The influence of stellar birth environment on protoplanetary disc dispersal.” 2019. Web. 20 Oct 2020.

Vancouver:

Winter A. The influence of stellar birth environment on protoplanetary disc dispersal. [Internet] [Doctoral dissertation]. University of Cambridge; 2019. [cited 2020 Oct 20]. Available from: https://www.repository.cam.ac.uk/handle/1810/293436.

Council of Science Editors:

Winter A. The influence of stellar birth environment on protoplanetary disc dispersal. [Doctoral Dissertation]. University of Cambridge; 2019. Available from: https://www.repository.cam.ac.uk/handle/1810/293436


University of Cambridge

15. Winter, Andrew. The influence of stellar birth environment on protoplanetary disc dispersal.

Degree: PhD, 2019, University of Cambridge

 Protoplanetary discs (PPDs) are the progenitors of planets and represent the material available for their formation. Recent surveys indicate that exoplanetary architectures are diverse and… (more)

Subjects/Keywords: Astronomy; Protoplanetary discs; Star formation; Planet formation; Stellar clusters; Exoplanets; accretion; accretion discs; circumstellar matter; Cygnus OB2; photoevaporation; tidal encounters; stellar dynamics; young stars

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APA (6th Edition):

Winter, A. (2019). The influence of stellar birth environment on protoplanetary disc dispersal. (Doctoral Dissertation). University of Cambridge. Retrieved from https://doi.org/10.17863/CAM.40585 ; https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.782773

Chicago Manual of Style (16th Edition):

Winter, Andrew. “The influence of stellar birth environment on protoplanetary disc dispersal.” 2019. Doctoral Dissertation, University of Cambridge. Accessed October 20, 2020. https://doi.org/10.17863/CAM.40585 ; https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.782773.

MLA Handbook (7th Edition):

Winter, Andrew. “The influence of stellar birth environment on protoplanetary disc dispersal.” 2019. Web. 20 Oct 2020.

Vancouver:

Winter A. The influence of stellar birth environment on protoplanetary disc dispersal. [Internet] [Doctoral dissertation]. University of Cambridge; 2019. [cited 2020 Oct 20]. Available from: https://doi.org/10.17863/CAM.40585 ; https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.782773.

Council of Science Editors:

Winter A. The influence of stellar birth environment on protoplanetary disc dispersal. [Doctoral Dissertation]. University of Cambridge; 2019. Available from: https://doi.org/10.17863/CAM.40585 ; https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.782773

16. Proszkow, Eva-Marie. Dynamical Evolution of Young Embedded Stellar Clusters: Environmental Effects on the Formation of Planetary Systems.

Degree: PhD, Physics, 2009, University of Michigan

 The dynamical evolution of young stellar clusters is studied to determine the effect cluster environment has on planetary formation in the disks surrounding cluster members.… (more)

Subjects/Keywords: Star Formation; Planet Formation; Stellar Clusters; Stellar Astrophysics; Numerical Simulations; Stellar Dynamics; Astronomy; Physics; Science

dynamics of embedded stellar clusters from the protocluster stage, through the embedded star… …near cluster centers). This chapter considers the dynamics of intermediate-sized stellar… …86 4.1 Stellar Distributions… …Distribution of ejection speeds for scattering interactions with central stellar mass M∗ = 0.50 M… …63 Distribution of ejection speeds for scattering interactions with central stellar mass M… 

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APA (6th Edition):

Proszkow, E. (2009). Dynamical Evolution of Young Embedded Stellar Clusters: Environmental Effects on the Formation of Planetary Systems. (Doctoral Dissertation). University of Michigan. Retrieved from http://hdl.handle.net/2027.42/63810

Chicago Manual of Style (16th Edition):

Proszkow, Eva-Marie. “Dynamical Evolution of Young Embedded Stellar Clusters: Environmental Effects on the Formation of Planetary Systems.” 2009. Doctoral Dissertation, University of Michigan. Accessed October 20, 2020. http://hdl.handle.net/2027.42/63810.

MLA Handbook (7th Edition):

Proszkow, Eva-Marie. “Dynamical Evolution of Young Embedded Stellar Clusters: Environmental Effects on the Formation of Planetary Systems.” 2009. Web. 20 Oct 2020.

Vancouver:

Proszkow E. Dynamical Evolution of Young Embedded Stellar Clusters: Environmental Effects on the Formation of Planetary Systems. [Internet] [Doctoral dissertation]. University of Michigan; 2009. [cited 2020 Oct 20]. Available from: http://hdl.handle.net/2027.42/63810.

Council of Science Editors:

Proszkow E. Dynamical Evolution of Young Embedded Stellar Clusters: Environmental Effects on the Formation of Planetary Systems. [Doctoral Dissertation]. University of Michigan; 2009. Available from: http://hdl.handle.net/2027.42/63810

17. Bruno, Giovanni. Characterization of transiting exoplanets : analyzing the impact of the host star on the planet parameters : Caractérisation d’exoplanètes en transit : analyse de l’impact de l’étoile hôte sur les paramètres de la planète.

Degree: Docteur es, Astrophysique et Cosmologie, 2015, Aix Marseille Université

Dans le cadre de ma thèse, j’ai analysé les spectres de neuf étoiles Kepler obtenus avec les relevés de vitesse radiale (VR). Cela a permis… (more)

Subjects/Keywords: Exoplanètes; Spectroscopie; Dynamique des systèemes multi-Planètaires; Transit; Activité stellaire; Exoplanets; Spectroscopy; Dynamics of multi-Planetary systems; Transit; Stellar activity

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APA (6th Edition):

Bruno, G. (2015). Characterization of transiting exoplanets : analyzing the impact of the host star on the planet parameters : Caractérisation d’exoplanètes en transit : analyse de l’impact de l’étoile hôte sur les paramètres de la planète. (Doctoral Dissertation). Aix Marseille Université. Retrieved from http://www.theses.fr/2015AIXM4746

Chicago Manual of Style (16th Edition):

Bruno, Giovanni. “Characterization of transiting exoplanets : analyzing the impact of the host star on the planet parameters : Caractérisation d’exoplanètes en transit : analyse de l’impact de l’étoile hôte sur les paramètres de la planète.” 2015. Doctoral Dissertation, Aix Marseille Université. Accessed October 20, 2020. http://www.theses.fr/2015AIXM4746.

MLA Handbook (7th Edition):

Bruno, Giovanni. “Characterization of transiting exoplanets : analyzing the impact of the host star on the planet parameters : Caractérisation d’exoplanètes en transit : analyse de l’impact de l’étoile hôte sur les paramètres de la planète.” 2015. Web. 20 Oct 2020.

Vancouver:

Bruno G. Characterization of transiting exoplanets : analyzing the impact of the host star on the planet parameters : Caractérisation d’exoplanètes en transit : analyse de l’impact de l’étoile hôte sur les paramètres de la planète. [Internet] [Doctoral dissertation]. Aix Marseille Université 2015. [cited 2020 Oct 20]. Available from: http://www.theses.fr/2015AIXM4746.

Council of Science Editors:

Bruno G. Characterization of transiting exoplanets : analyzing the impact of the host star on the planet parameters : Caractérisation d’exoplanètes en transit : analyse de l’impact de l’étoile hôte sur les paramètres de la planète. [Doctoral Dissertation]. Aix Marseille Université 2015. Available from: http://www.theses.fr/2015AIXM4746


University of Oxford

18. Williams, Michael J. Early-type disk galaxies.

Degree: PhD, 2011, University of Oxford

 In this thesis I investigate the dynamics and stellar populations of a sample of 28 edge-on early-type (S0 – Sb) disk galaxies, 22 of which host… (more)

Subjects/Keywords: 520; Astrophysics; galaxies; early-type; spiral; s0; dynamics; kinematics; bulge; disk; stellar populations; bars; galaxy evolution; galaxy formation

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APA (6th Edition):

Williams, M. J. (2011). Early-type disk galaxies. (Doctoral Dissertation). University of Oxford. Retrieved from http://ora.ox.ac.uk/objects/uuid:936168ab-f49a-410a-9e1b-80c7ad7cf556 ; https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.540277

Chicago Manual of Style (16th Edition):

Williams, Michael J. “Early-type disk galaxies.” 2011. Doctoral Dissertation, University of Oxford. Accessed October 20, 2020. http://ora.ox.ac.uk/objects/uuid:936168ab-f49a-410a-9e1b-80c7ad7cf556 ; https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.540277.

MLA Handbook (7th Edition):

Williams, Michael J. “Early-type disk galaxies.” 2011. Web. 20 Oct 2020.

Vancouver:

Williams MJ. Early-type disk galaxies. [Internet] [Doctoral dissertation]. University of Oxford; 2011. [cited 2020 Oct 20]. Available from: http://ora.ox.ac.uk/objects/uuid:936168ab-f49a-410a-9e1b-80c7ad7cf556 ; https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.540277.

Council of Science Editors:

Williams MJ. Early-type disk galaxies. [Doctoral Dissertation]. University of Oxford; 2011. Available from: http://ora.ox.ac.uk/objects/uuid:936168ab-f49a-410a-9e1b-80c7ad7cf556 ; https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.540277

19. Sande, Jesse van de. Dawn of the red and dead: stellar kinematics of massive quiescent galaxies out to z = 2.

Degree: 2014, Leiden Observatory, Faculty of Science, Leiden University

 The first massive elliptical galaxies were already in place when the Universe was only 3 billions years old. Surprisingly, they are more compact in comparison… (more)

Subjects/Keywords: Galaxies: evolution; Formation; Kinematics; Dynamics; Stellar content; Structure; Galaxies: evolution; Formation; Kinematics; Dynamics; Stellar content; Structure

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APA (6th Edition):

Sande, J. v. d. (2014). Dawn of the red and dead: stellar kinematics of massive quiescent galaxies out to z = 2. (Doctoral Dissertation). Leiden Observatory, Faculty of Science, Leiden University. Retrieved from http://hdl.handle.net/1887/28962

Chicago Manual of Style (16th Edition):

Sande, Jesse van de. “Dawn of the red and dead: stellar kinematics of massive quiescent galaxies out to z = 2.” 2014. Doctoral Dissertation, Leiden Observatory, Faculty of Science, Leiden University. Accessed October 20, 2020. http://hdl.handle.net/1887/28962.

MLA Handbook (7th Edition):

Sande, Jesse van de. “Dawn of the red and dead: stellar kinematics of massive quiescent galaxies out to z = 2.” 2014. Web. 20 Oct 2020.

Vancouver:

Sande Jvd. Dawn of the red and dead: stellar kinematics of massive quiescent galaxies out to z = 2. [Internet] [Doctoral dissertation]. Leiden Observatory, Faculty of Science, Leiden University; 2014. [cited 2020 Oct 20]. Available from: http://hdl.handle.net/1887/28962.

Council of Science Editors:

Sande Jvd. Dawn of the red and dead: stellar kinematics of massive quiescent galaxies out to z = 2. [Doctoral Dissertation]. Leiden Observatory, Faculty of Science, Leiden University; 2014. Available from: http://hdl.handle.net/1887/28962

20. Ochsendorf, Bram Benjamin. Tales of Orion: the interplay of gas, dust, and stars in the interstellar medium.

Degree: 2015, Leiden Observatory, Faculty of Science, Leiden University

 The space between stars is filled with a dilute mixture of atoms, molecules, and dust grains, which we call the interstellar medium (ISM). The physics… (more)

Subjects/Keywords: Interstellar medium; HII regions; Super(bubbles); Dust; Dynamics; Stellar feedback; Interstellar medium; HII regions; Super(bubbles); Dust; Dynamics; Stellar feedback

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APA (6th Edition):

Ochsendorf, B. B. (2015). Tales of Orion: the interplay of gas, dust, and stars in the interstellar medium. (Doctoral Dissertation). Leiden Observatory, Faculty of Science, Leiden University. Retrieved from http://hdl.handle.net/1887/34931

Chicago Manual of Style (16th Edition):

Ochsendorf, Bram Benjamin. “Tales of Orion: the interplay of gas, dust, and stars in the interstellar medium.” 2015. Doctoral Dissertation, Leiden Observatory, Faculty of Science, Leiden University. Accessed October 20, 2020. http://hdl.handle.net/1887/34931.

MLA Handbook (7th Edition):

Ochsendorf, Bram Benjamin. “Tales of Orion: the interplay of gas, dust, and stars in the interstellar medium.” 2015. Web. 20 Oct 2020.

Vancouver:

Ochsendorf BB. Tales of Orion: the interplay of gas, dust, and stars in the interstellar medium. [Internet] [Doctoral dissertation]. Leiden Observatory, Faculty of Science, Leiden University; 2015. [cited 2020 Oct 20]. Available from: http://hdl.handle.net/1887/34931.

Council of Science Editors:

Ochsendorf BB. Tales of Orion: the interplay of gas, dust, and stars in the interstellar medium. [Doctoral Dissertation]. Leiden Observatory, Faculty of Science, Leiden University; 2015. Available from: http://hdl.handle.net/1887/34931


Macquarie University

21. Smith, Ian Lindsay. An analysis of HCN observations of the galactic centre's Circumnuclear Disk.

Degree: MPhil, 2012, Macquarie University

Bibliography: p. 93-96.

The Circumnuclear Disk  – Molecular excitation, line formation and radiative transfer  – Disk geometry, HCN cores and masers  – Analysis of HCN… (more)

Subjects/Keywords: Disks (Astrophysics); Circumstellar matter; Interstellar hydrogen; Gas dynamics  – Mathematical models; Interstellar molecules; Stellar dynamics; Black holes (Astronomy); Hydrocyanic acid gas; Galactic center; galactic centre; Circumnuclear Disk; HCN

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APA (6th Edition):

Smith, I. L. (2012). An analysis of HCN observations of the galactic centre's Circumnuclear Disk. (Masters Thesis). Macquarie University. Retrieved from http://hdl.handle.net/1959.14/1276227

Chicago Manual of Style (16th Edition):

Smith, Ian Lindsay. “An analysis of HCN observations of the galactic centre's Circumnuclear Disk.” 2012. Masters Thesis, Macquarie University. Accessed October 20, 2020. http://hdl.handle.net/1959.14/1276227.

MLA Handbook (7th Edition):

Smith, Ian Lindsay. “An analysis of HCN observations of the galactic centre's Circumnuclear Disk.” 2012. Web. 20 Oct 2020.

Vancouver:

Smith IL. An analysis of HCN observations of the galactic centre's Circumnuclear Disk. [Internet] [Masters thesis]. Macquarie University; 2012. [cited 2020 Oct 20]. Available from: http://hdl.handle.net/1959.14/1276227.

Council of Science Editors:

Smith IL. An analysis of HCN observations of the galactic centre's Circumnuclear Disk. [Masters Thesis]. Macquarie University; 2012. Available from: http://hdl.handle.net/1959.14/1276227


Ohio University

22. Salow, Robert M. Self-Gravitating Eccentric Disk Models for the Double Nucleus of Μ31.

Degree: PhD, Physics (Arts and Sciences), 2004, Ohio University

  We present new dynamical models of weakly self-gravitating, finite dispersion eccentric stellar disks around central black holes for the double nucleus of Μ31. The… (more)

Subjects/Keywords: Physics, Astronomy and Astrophysics; Black Holes; Galaxy Nuclei; Galactic Dynamics; Stellar Dynamics

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APA (6th Edition):

Salow, R. M. (2004). Self-Gravitating Eccentric Disk Models for the Double Nucleus of Μ31. (Doctoral Dissertation). Ohio University. Retrieved from http://rave.ohiolink.edu/etdc/view?acc_num=ohiou1088521276

Chicago Manual of Style (16th Edition):

Salow, Robert M. “Self-Gravitating Eccentric Disk Models for the Double Nucleus of Μ31.” 2004. Doctoral Dissertation, Ohio University. Accessed October 20, 2020. http://rave.ohiolink.edu/etdc/view?acc_num=ohiou1088521276.

MLA Handbook (7th Edition):

Salow, Robert M. “Self-Gravitating Eccentric Disk Models for the Double Nucleus of Μ31.” 2004. Web. 20 Oct 2020.

Vancouver:

Salow RM. Self-Gravitating Eccentric Disk Models for the Double Nucleus of Μ31. [Internet] [Doctoral dissertation]. Ohio University; 2004. [cited 2020 Oct 20]. Available from: http://rave.ohiolink.edu/etdc/view?acc_num=ohiou1088521276.

Council of Science Editors:

Salow RM. Self-Gravitating Eccentric Disk Models for the Double Nucleus of Μ31. [Doctoral Dissertation]. Ohio University; 2004. Available from: http://rave.ohiolink.edu/etdc/view?acc_num=ohiou1088521276

23. Boekholt, Tjarda Coenraad Nico. Chaotic dynamics in N-body systems.

Degree: 2015, Leiden Observatory, Faculty of Science, Leiden University

 Ever since Isaac Newton in 1687 posed the N-body problem, astronomers have been looking for its solutions in order to understand the evolution of dynamical… (more)

Subjects/Keywords: Planetary dynamics; Stellar dynamics; Comet Halley; N-body problem; Numerical methods; Planetary dynamics; Stellar dynamics; Comet Halley; N-body problem; Numerical methods

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APA (6th Edition):

Boekholt, T. C. N. (2015). Chaotic dynamics in N-body systems. (Doctoral Dissertation). Leiden Observatory, Faculty of Science, Leiden University. Retrieved from http://hdl.handle.net/1887/36077

Chicago Manual of Style (16th Edition):

Boekholt, Tjarda Coenraad Nico. “Chaotic dynamics in N-body systems.” 2015. Doctoral Dissertation, Leiden Observatory, Faculty of Science, Leiden University. Accessed October 20, 2020. http://hdl.handle.net/1887/36077.

MLA Handbook (7th Edition):

Boekholt, Tjarda Coenraad Nico. “Chaotic dynamics in N-body systems.” 2015. Web. 20 Oct 2020.

Vancouver:

Boekholt TCN. Chaotic dynamics in N-body systems. [Internet] [Doctoral dissertation]. Leiden Observatory, Faculty of Science, Leiden University; 2015. [cited 2020 Oct 20]. Available from: http://hdl.handle.net/1887/36077.

Council of Science Editors:

Boekholt TCN. Chaotic dynamics in N-body systems. [Doctoral Dissertation]. Leiden Observatory, Faculty of Science, Leiden University; 2015. Available from: http://hdl.handle.net/1887/36077


Universiteit Utrecht

24. Hamers, A.S. The evolution of coeval stellar hierarchical triple systems.

Degree: 2012, Universiteit Utrecht

 We study the evolution of coeval stellar hierarchical triple systems with intermediate mass (initial primary mass 1.0 < m1 /Msun < 6.5) and relatively wide… (more)

Subjects/Keywords: celestial mechanics; hierarchical triple systems; triple stars; triple dynamics; stellar evolution; triple population synthesis; carbon oxygen white dwarf mergers; supernovae type Ia

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APA (6th Edition):

Hamers, A. S. (2012). The evolution of coeval stellar hierarchical triple systems. (Masters Thesis). Universiteit Utrecht. Retrieved from http://dspace.library.uu.nl:8080/handle/1874/253221

Chicago Manual of Style (16th Edition):

Hamers, A S. “The evolution of coeval stellar hierarchical triple systems.” 2012. Masters Thesis, Universiteit Utrecht. Accessed October 20, 2020. http://dspace.library.uu.nl:8080/handle/1874/253221.

MLA Handbook (7th Edition):

Hamers, A S. “The evolution of coeval stellar hierarchical triple systems.” 2012. Web. 20 Oct 2020.

Vancouver:

Hamers AS. The evolution of coeval stellar hierarchical triple systems. [Internet] [Masters thesis]. Universiteit Utrecht; 2012. [cited 2020 Oct 20]. Available from: http://dspace.library.uu.nl:8080/handle/1874/253221.

Council of Science Editors:

Hamers AS. The evolution of coeval stellar hierarchical triple systems. [Masters Thesis]. Universiteit Utrecht; 2012. Available from: http://dspace.library.uu.nl:8080/handle/1874/253221


Universidade do Rio Grande do Sul

25. Ferrari, Guilherme Gonçalves. Novos mapas simpléticos para integração de sistemas hamiltonianos com múltiplas escalas de tempo : enfoque em sistemas gravitacionais de N-corpos.

Degree: 2015, Universidade do Rio Grande do Sul

Mapas simpléticos são bem conhecidos por preservarem o volume do espaço de fase em dinâmica Hamiltoniana e são particularmente apropriados para problemas que requerem longos… (more)

Subjects/Keywords: Astrofisica; Stellar dynamics; Computação astronômica; N-body simulations; Integração numérica; Symplectic maps; Numerical integration; Sistemas hamiltonianos; Simulação computacional; GPGPU; Ondas gravitacionais; Dinamica estelar

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APA (6th Edition):

Ferrari, G. G. (2015). Novos mapas simpléticos para integração de sistemas hamiltonianos com múltiplas escalas de tempo : enfoque em sistemas gravitacionais de N-corpos. (Thesis). Universidade do Rio Grande do Sul. Retrieved from http://hdl.handle.net/10183/127985

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):

Ferrari, Guilherme Gonçalves. “Novos mapas simpléticos para integração de sistemas hamiltonianos com múltiplas escalas de tempo : enfoque em sistemas gravitacionais de N-corpos.” 2015. Thesis, Universidade do Rio Grande do Sul. Accessed October 20, 2020. http://hdl.handle.net/10183/127985.

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

MLA Handbook (7th Edition):

Ferrari, Guilherme Gonçalves. “Novos mapas simpléticos para integração de sistemas hamiltonianos com múltiplas escalas de tempo : enfoque em sistemas gravitacionais de N-corpos.” 2015. Web. 20 Oct 2020.

Vancouver:

Ferrari GG. Novos mapas simpléticos para integração de sistemas hamiltonianos com múltiplas escalas de tempo : enfoque em sistemas gravitacionais de N-corpos. [Internet] [Thesis]. Universidade do Rio Grande do Sul; 2015. [cited 2020 Oct 20]. Available from: http://hdl.handle.net/10183/127985.

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

Council of Science Editors:

Ferrari GG. Novos mapas simpléticos para integração de sistemas hamiltonianos com múltiplas escalas de tempo : enfoque em sistemas gravitacionais de N-corpos. [Thesis]. Universidade do Rio Grande do Sul; 2015. Available from: http://hdl.handle.net/10183/127985

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

26. Yelda, Sylvana. Constraining the Recent Star Formation History of the Galactic Center with High Precision Astrometry.

Degree: Astronomy, 2012, UCLA

 The proximity of the Galactic center has allowed for the detailed study of the environs of a supermassive black hole (SMBH). While the region is… (more)

Subjects/Keywords: Astrophysics; astrometry; high angular resolution; infrared; stars; stellar dynamics

…about stellar dynamics. Thank you, Rainer Schoedel, for your long-distance support and… …stellar dynamics near a supermassive black hole (SMBH). At a distance of 8 kpc, the… …59 Motion of the Central Stellar Cluster in a Sgr A* Rest Frame 66 2.4 Summary… …Distribution and Radial Structure of the Young Stellar Disk in the Galactic Center… …Eccentricity Distribution of the Clockwise Disk Stars . . . 119 3.5.4 3.6 Stellar Orbits… 

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APA (6th Edition):

Yelda, S. (2012). Constraining the Recent Star Formation History of the Galactic Center with High Precision Astrometry. (Thesis). UCLA. Retrieved from http://www.escholarship.org/uc/item/9ts8f6c8

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):

Yelda, Sylvana. “Constraining the Recent Star Formation History of the Galactic Center with High Precision Astrometry.” 2012. Thesis, UCLA. Accessed October 20, 2020. http://www.escholarship.org/uc/item/9ts8f6c8.

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

MLA Handbook (7th Edition):

Yelda, Sylvana. “Constraining the Recent Star Formation History of the Galactic Center with High Precision Astrometry.” 2012. Web. 20 Oct 2020.

Vancouver:

Yelda S. Constraining the Recent Star Formation History of the Galactic Center with High Precision Astrometry. [Internet] [Thesis]. UCLA; 2012. [cited 2020 Oct 20]. Available from: http://www.escholarship.org/uc/item/9ts8f6c8.

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

Council of Science Editors:

Yelda S. Constraining the Recent Star Formation History of the Galactic Center with High Precision Astrometry. [Thesis]. UCLA; 2012. Available from: http://www.escholarship.org/uc/item/9ts8f6c8

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


Macquarie University

27. Conn, Anthony Rhys. Structure of the M31 satellite system: Bayesian distances from the tip of the Red Giant Branch.

Degree: 2013, Macquarie University

Thesis by publication.

"A thesis completed under a cotutelle agreement between Macquarie University and the Université de Strasbourg for the degree of Doctor of Philosophy… (more)

Subjects/Keywords: Galaxies  – Evolution; Galactic dynamics; Andromeda Galaxy; satellite galaxies; M31 (Galaxy); galaxies: general; galaxies: stellar content; galaxies: dwarf; galaxies: halos; galaxies: individual (M31); galaxies: structure; local group

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APA (6th Edition):

Conn, A. R. (2013). Structure of the M31 satellite system: Bayesian distances from the tip of the Red Giant Branch. (Doctoral Dissertation). Macquarie University. Retrieved from http://hdl.handle.net/1959.14/1264793

Chicago Manual of Style (16th Edition):

Conn, Anthony Rhys. “Structure of the M31 satellite system: Bayesian distances from the tip of the Red Giant Branch.” 2013. Doctoral Dissertation, Macquarie University. Accessed October 20, 2020. http://hdl.handle.net/1959.14/1264793.

MLA Handbook (7th Edition):

Conn, Anthony Rhys. “Structure of the M31 satellite system: Bayesian distances from the tip of the Red Giant Branch.” 2013. Web. 20 Oct 2020.

Vancouver:

Conn AR. Structure of the M31 satellite system: Bayesian distances from the tip of the Red Giant Branch. [Internet] [Doctoral dissertation]. Macquarie University; 2013. [cited 2020 Oct 20]. Available from: http://hdl.handle.net/1959.14/1264793.

Council of Science Editors:

Conn AR. Structure of the M31 satellite system: Bayesian distances from the tip of the Red Giant Branch. [Doctoral Dissertation]. Macquarie University; 2013. Available from: http://hdl.handle.net/1959.14/1264793

28. A. Zocchi. OBSERVATIONAL TESTS ON THE DYNAMICS OF GLOBULAR CLUSTERS.

Degree: 2014, Università degli Studi di Milano

 Galactic globular clusters are nearly gas-free, self-gravitating stellar systems characterized by an apparently simple geometry, with finite size probably determined by tidal truncation. These unique… (more)

Subjects/Keywords: stellar dynamics and kinematics; stellar clusters and associations; globular clusters in the milky way; Settore FIS/05 - Astronomia e Astrofisica

…them excellent laboratories for studies of stellar dynamics, and ideal targets for N-body… …describe the dynamics of a stellar system. Chapter 3: Observations and model testing: We give an… …simulated isolated cluster with stellar evolution. Properties of the samples. Dimensionless… …models. Derived parameters for the isolated cluster with stellar evolution. Derived parameters… …are nearly gas-free, self-gravitating stellar systems characterized by an apparently simple… 

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APA (6th Edition):

Zocchi, A. (2014). OBSERVATIONAL TESTS ON THE DYNAMICS OF GLOBULAR CLUSTERS. (Thesis). Università degli Studi di Milano. Retrieved from http://hdl.handle.net/2434/235122

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):

Zocchi, A.. “OBSERVATIONAL TESTS ON THE DYNAMICS OF GLOBULAR CLUSTERS.” 2014. Thesis, Università degli Studi di Milano. Accessed October 20, 2020. http://hdl.handle.net/2434/235122.

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

MLA Handbook (7th Edition):

Zocchi, A.. “OBSERVATIONAL TESTS ON THE DYNAMICS OF GLOBULAR CLUSTERS.” 2014. Web. 20 Oct 2020.

Vancouver:

Zocchi A. OBSERVATIONAL TESTS ON THE DYNAMICS OF GLOBULAR CLUSTERS. [Internet] [Thesis]. Università degli Studi di Milano; 2014. [cited 2020 Oct 20]. Available from: http://hdl.handle.net/2434/235122.

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

Council of Science Editors:

Zocchi A. OBSERVATIONAL TESTS ON THE DYNAMICS OF GLOBULAR CLUSTERS. [Thesis]. Università degli Studi di Milano; 2014. Available from: http://hdl.handle.net/2434/235122

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

29. Brown, Justin. The Effects of Small-Scale Mixing Processes on Supernova Progenitors.

Degree: Astronomy & Astrophysics, 2016, University of California – Santa Cruz

 Minor mixing processes—any fluid processes that mix material or transport heat other than convection or other large-scale flows—play a critical role in stellar evolution. These… (more)

Subjects/Keywords: Astronomy; Astrophysics; Applied mathematics; computational fluid dynamics; massive stars; overshooting convection; semiconvection; stellar evolution; thermohaline convection

…combination of neutrinos and helium burning. Stellar winds of all models have been included… …the stellar lifetime, using the depletion of hydrogen on the main sequence (top left… …and a hydrogen burning shell that are separated by a few numerical cells. Because stellar… …fraction of stellar material, it is unlikely that this is a physical effect. The only way to… …a red or blue supergiant is an observable diagnostic of stellar evolution as it can be… 

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

APA (6th Edition):

Brown, J. (2016). The Effects of Small-Scale Mixing Processes on Supernova Progenitors. (Thesis). University of California – Santa Cruz. Retrieved from http://www.escholarship.org/uc/item/7xf9x6vk

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):

Brown, Justin. “The Effects of Small-Scale Mixing Processes on Supernova Progenitors.” 2016. Thesis, University of California – Santa Cruz. Accessed October 20, 2020. http://www.escholarship.org/uc/item/7xf9x6vk.

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

MLA Handbook (7th Edition):

Brown, Justin. “The Effects of Small-Scale Mixing Processes on Supernova Progenitors.” 2016. Web. 20 Oct 2020.

Vancouver:

Brown J. The Effects of Small-Scale Mixing Processes on Supernova Progenitors. [Internet] [Thesis]. University of California – Santa Cruz; 2016. [cited 2020 Oct 20]. Available from: http://www.escholarship.org/uc/item/7xf9x6vk.

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

Council of Science Editors:

Brown J. The Effects of Small-Scale Mixing Processes on Supernova Progenitors. [Thesis]. University of California – Santa Cruz; 2016. Available from: http://www.escholarship.org/uc/item/7xf9x6vk

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

30. Leaman, Ryan. Constraints on environmental and secular effects on the chemodynamical evolution of dwarf galaxies.

Degree: Dept. of Physics and Astronomy, 2012, University of Victoria

 This thesis presents observations and analysis relating to the understanding of processes that govern the formation and evolution of low mass galactic systems. In particular… (more)

Subjects/Keywords: Astrophysics; Galaxy Evolution and Formation; Galaxy Dynamics; Chemical Evolution of Galaxies; Stellar Populations

…Gaseous and Stellar Velocity Fields . . . . . . . . . . . . . . . . . . . 30 2.8 WLM Optical… …37 2.11 Photometric Position Angles and Ellipticities for Gaseous and Stellar Populations… …38 2.12 Major Axis Gaseous and Stellar Velocity Profile . . . . . . . . . . . . 40 2.13… …Gaseous and Stellar Populations . . . . 45 2.16 Observed and Intrinsic Axial Ratios… …vs. Half Light Radius for Local Group Dwarfs . . . . . . . 55 2.20 Stellar Velocity… 

Record DetailsSimilar RecordsGoogle PlusoneFacebookTwitterCiteULikeMendeleyreddit

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

APA (6th Edition):

Leaman, R. (2012). Constraints on environmental and secular effects on the chemodynamical evolution of dwarf galaxies. (Thesis). University of Victoria. Retrieved from http://hdl.handle.net/1828/4070

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):

Leaman, Ryan. “Constraints on environmental and secular effects on the chemodynamical evolution of dwarf galaxies.” 2012. Thesis, University of Victoria. Accessed October 20, 2020. http://hdl.handle.net/1828/4070.

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

MLA Handbook (7th Edition):

Leaman, Ryan. “Constraints on environmental and secular effects on the chemodynamical evolution of dwarf galaxies.” 2012. Web. 20 Oct 2020.

Vancouver:

Leaman R. Constraints on environmental and secular effects on the chemodynamical evolution of dwarf galaxies. [Internet] [Thesis]. University of Victoria; 2012. [cited 2020 Oct 20]. Available from: http://hdl.handle.net/1828/4070.

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

Council of Science Editors:

Leaman R. Constraints on environmental and secular effects on the chemodynamical evolution of dwarf galaxies. [Thesis]. University of Victoria; 2012. Available from: http://hdl.handle.net/1828/4070

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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