Mass-radius relations for massive white dwarf stars

We present detailed theoretical mass-radius relations for massive white dwarf stars with oxygen-neon cores. This work is motivated by recent observational evidence about the existence of white dwarf stars with very high surface gravities. Our results are based on evolutionary calculations that take...

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Detalles Bibliográficos
Autores principales:	Althaus, Leandro Gabriel, García Berro, E., Isern, J., Córsico, Alejandro Hugo
Formato:	Articulo
Lenguaje:	Inglés
Publicado:	2005
Materias:	Ciencias Astronómicas Stars: evolution Stars: fundamental parameters Stars: white dwarfs
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/83529
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

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