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Photometric and Spectroscopic Monitoring of the SDBV Star PG 1605+072:
A small fraction of sdB stars show short-period, multiperiodic light variations and form the new class of pulsating star known as EC 14026 variables, after the prototype, or, alternately, as sdBV stars. Until ...
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Chapter
Towards Asteroseismology of the Non-Radial Pulsating SDB Star PG 1605+072
The recently discovered new class of sdB pulsators (sdBV) offers a powerful possibility for the investigation of their interior and thus their evolutionary history. The first step towards applying asteroseismo...