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2011CoAst.162...73L - Com. in Asteroseismology, 162, 73 (2011/July-0)
New pulsation analysis of the oscillating eclipsing binary BG Peg.
LIAKOS A. and NIARCHOS P.
Abstract (from CDS):
New BVRI light curves of the eclipsing binary BG Peg were obtained and analysed using the Wilson-Devinney code. The observations (102 hours during a span of 108 days) were collected to perform an accurate frequency analysis of the pulsations of the primary component of the system, which is of Delta Sct type. Three pulsation frequencies were identified in that star.
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Simbad objects: 1
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