Axially Symmetric Post-Newtonian Stellar Systems

Axially Symmetric Post-Newtonian Stellar Systems

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We introduce a method to obtain self-consistent, axially symmetric disklike stellar models in the first post-Newtonian (1PN) approximation. By using in the field equations of the 1PN approximation a distribution function (DF) corresponding to a Newtonian model, two fundamental equations determin...

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Bibliographic Details
Main Authors: Camilo Akímushkin, Javier Ramos-Caro, Guillermo A. González
Format: Article
Language:Spanish
Published: Universidad Industrial de Santander 2010-06-01
Series:Revista Integración
Subjects:
Post-Newtonian approximation
galactic and stellar dynamics
galactic
stellar dynamics
Primer aproximación post-newtoniana
dinámicas estelar
galáctica
Online Access:http://revistas.uis.edu.co/index.php/revistaintegracion/article/view/2056/2418

Internet

http://revistas.uis.edu.co/index.php/revistaintegracion/article/view/2056/2418

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