A Convective Model for Light Curves of ZZ Ceti Stars

Details A Convective Model for Light Curves of ZZ Ceti Stars A Convective Model for Light Curves of ZZ Ceti Stars

Jul 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aspc..334..593f&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 erratic behavior of the luminosity in ZZ Ceti light curves may be
explained in terms of the sum of several convective fluctuations, where
the heat flux is propagated in time by thermal waves. We present
simulations of the light curves of GD29-38, GD 358, and HL Tau-76.

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