The ages and colours of cool helium-core white dwarf stars

The purpose of this work is to explore the evolution of helium-core white dwarf stars in a self-consistent way with the predictions of detailed non-grey model atmospheres and element diffusion. To this end, we consider helium-core white dwarf models with stellar masses of 0.406, 0.360, 0.327, 0.292,...

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Detalles Bibliográficos
Autores principales: Serenelli, Aldo Marcelo, Althaus, Leandro Gabriel, Benvenuto, Omar Gustavo
Formato: Articulo
Lenguaje:Inglés
Publicado: 2001
Materias:
Ciencias Astronómicas
stars: atmospheres
stars: evolution
stars: fundamental parameters
stars: interiors
white dwarfs
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/2055
http://fcaglp.fcaglp.unlp.edu.ar/evolgroup/Papers/ARTICLES/2001/MNRAS_325_607_2001.pdf
http://mnras.oxfordjournals.org/content/325/2/607
Aporte de:
SEDICI (UNLP) de Universidad Nacional de La Plata

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