Classical and post-newtonian model of X-ray burster

The thermo-mechanical oscillations of a radiating spherical shell are studied. With a reasonable choice of the parameters the simple model reproduces the behaviour of X-ray bursters and recurrent novae. Different hypothesis on the radiation pressure are introduced and the problem is studied at the c...

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Detalles Bibliográficos
Autores principales: Aquilano, R. O., Castagnino, M. A., Lara, L.
Formato: Articulo Comunicacion
Lenguaje:Español
Publicado: 1988
Materias:
Astronomía
Galaxia
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/141977
Aporte de:
SEDICI (UNLP) de Universidad Nacional de La Plata
id I19-R120-10915-141977
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spelling I19-R120-10915-1419772024-09-10T18:50:15Z http://sedici.unlp.edu.ar/handle/10915/141977 Classical and post-newtonian model of X-ray burster Aquilano, R. O. Castagnino, M. A. Lara, L. 1988 2022-09-13T13:34:47Z es Astronomía Galaxia The thermo-mechanical oscillations of a radiating spherical shell are studied. With a reasonable choice of the parameters the simple model reproduces the behaviour of X-ray bursters and recurrent novae. Different hypothesis on the radiation pressure are introduced and the problem is studied at the classical and post-newtonian levels. Asociación Argentina de Astronomía Articulo Comunicacion http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) application/pdf
institution Universidad Nacional de La Plata
institution_str I-19
repository_str R-120
collection SEDICI (UNLP)
language Español
topic Astronomía
Galaxia
spellingShingle Astronomía
Galaxia
Aquilano, R. O.
Castagnino, M. A.
Lara, L.
Classical and post-newtonian model of X-ray burster
topic_facet Astronomía
Galaxia
description The thermo-mechanical oscillations of a radiating spherical shell are studied. With a reasonable choice of the parameters the simple model reproduces the behaviour of X-ray bursters and recurrent novae. Different hypothesis on the radiation pressure are introduced and the problem is studied at the classical and post-newtonian levels.
format Articulo
Comunicacion
author Aquilano, R. O.
Castagnino, M. A.
Lara, L.
author_facet Aquilano, R. O.
Castagnino, M. A.
Lara, L.
author_sort Aquilano, R. O.
title Classical and post-newtonian model of X-ray burster
title_short Classical and post-newtonian model of X-ray burster
title_full Classical and post-newtonian model of X-ray burster
title_fullStr Classical and post-newtonian model of X-ray burster
title_full_unstemmed Classical and post-newtonian model of X-ray burster
title_sort classical and post-newtonian model of x-ray burster
publishDate 1988
url http://sedici.unlp.edu.ar/handle/10915/141977
work_keys_str_mv AT aquilanoro classicalandpostnewtonianmodelofxrayburster
AT castagninoma classicalandpostnewtonianmodelofxrayburster
AT laral classicalandpostnewtonianmodelofxrayburster
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