White Dwarf Cooling by Means of Heat Waves

Details White Dwarf Cooling by Means of Heat Waves White Dwarf Cooling by Means of Heat Waves

Jul 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aspc..334...69f&link_type=abstract

14th European Workshop on White Dwarfs, ASP Conference Series, Vol. 334 Proceedings of a meeting held at Kiel, July 19-23, 2004

Astronomy and Astrophysics

Astronomy

Scientific paper

The standard white dwarf (WD) cooling theory is revised when the heat
flux is propagate by thermal waves in degenerate material. Before the
relaxation time, the luminosity function is dampening oscillation and
the WD-age increase.

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