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Paper: Pulsating Subdwarf B Stars in Close Binaries
Volume: 334, 14th European Workshop on White Dwarfs
Page: 607
Authors: Reed, M.D.; Brondel, B.J.
Abstract: 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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