C/O white dwarfs of very low mass: 0.33-0.5 Mo
Astrophysics
2009-07-22 v1
Abstract
The standard lower limit for the mass of white dwarfs (WDs) with a C/O core is roughly 0.5 Mo. In the present work we investigated the possibility to form C/O WDs with mass as low as 0.33 Mo. Both the pre-WD and the cooling evolution of such nonstandard models will be described.
Cite
@article{arxiv.0812.3729,
title = {C/O white dwarfs of very low mass: 0.33-0.5 Mo},
author = {P. G. Prada Moroni and O. Straniero},
journal= {arXiv preprint arXiv:0812.3729},
year = {2009}
}
Comments
Submitted to the "Proceedings of the 16th European White Dwarf Workshop" (to be published JPCS). 7 pages including 13 figures