Computer Science
Scientific paper
Jan 2007
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007ycat..34650249a&link_type=abstract
VizieR On-line Data Catalog: J/A+A/465/249. Originally published in: 2007A&A...465..249A
Computer Science
Stars: White Dwarf, Models: Atmosphere, Stars: Ages, Photometry
Scientific paper
We present evolutionary calculations and colors for massive white dwarfs with oxygen-neon cores for masses between 1.06 and 1.28M{sun}. The evolutionary stages computed cover the luminosity range from log(L/L{sun})~0.5 down to -5.2. Our cooling sequences are based on evolutionary calculations that take into account the chemical composition expected from massive white dwarf progenitors that burned carbon in partially degenerate conditions. The use of detailed non-gray model atmospheres provides us with accurate outer boundary conditions for our evolving models at low effective temperatures.
(1 data file).
Althaus Leandro G.
Corsico Alejandro
Garcia-Berro Enrique
Isern Jordi
Rohrmann R.
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