New pulsation analysis of the oscillating Eclipsing Binary BG Peg

Details New pulsation analysis of the oscillating Eclipsing Binary BG Peg New pulsation analysis of the oscillating Eclipsing Binary BG Peg

Jul 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011coast.162...73l&link_type=abstract

Communications in Asteroseismology, Vol. 162, p. 73

Computer Science

1

Scientific paper

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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