Pulsating Subdwarf B Stars in Close Binaries

Details Pulsating Subdwarf B Stars in Close Binaries Pulsating Subdwarf B Stars in Close Binaries

Jul 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aspc..334..607r&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

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Scientific paper

Asteroseismology has successfully been applied to our Sun, white dwarfs, Cepheids and a few other classes of variable stars. The successful application of asteroseismology depends on the determination of the pulsation spherical harmonics, a task that has largely been unsuccessful in pulsating subdwarf B stars. In this paper, we investigate pulsating subdwarf B stars in close binaries as a useful tool for identifying pulsation modes.

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