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Axially Symmetric Post-Newtonian Stellar Systems
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 determining...
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| Publicado no: | Revista Integración |
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| Main Authors: | , , |
| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado em: |
Universidad Industrial de Santander
2010
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| Assuntos: | |
| Acesso em linha: | https://www.redalyc.org/articulo.oa?id=327028017001 |
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