The ages and colours of cool helium-core white dwarf stars
Blue dwarf
Black dwarf
DOI:
10.1046/j.1365-8711.2001.04449.x
Publication Date:
2003-03-12T13:40:46Z
AUTHORS (4)
ABSTRACT
The purpose of this work is to explore the evolution helium-core white dwarf stars in a self-consistent way with predictions detailed non-grey model atmospheres and element diffusion. To end, we consider models stellar masses 0.406, 0.360, 0.327, 0.292, 0.242, 0.196 0.169 M⊙ follow their from end mass-loss episodes, during pre-white evolution, down very low surface luminosities.
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