White dwarfs of very low mass with C/O core

Details White dwarfs of very low mass with C/O core White dwarfs of very low mass with C/O core

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aipc.1111...63m&link_type=abstract

PROBING STELLAR POPULATIONS OUT TO THE DISTANT UNIVERSE: CEFALU 2008, Proceedings of the International Conference. AIP Conferen

Physics

2

Faint Blue Stars, White Dwarfs, Degenerate Stars, Nuclei Of Planetary Nebulae, Star Formation, Distances, Redshifts, Radial Velocities, Spatial Distribution Of Galaxies

Scientific paper

It is commonly believed that white dwarfs (WDs) with a carbon-oxygen
core must have mass larger than about 0.5Msolar. We will
discuss a possible scenario for the formation of C/O WDs with mass as
low as 0.33Msolar. A description of both the pre-WD and the
cooling evolution of such models of very low mass will be presented.

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