New pulsation analysis of the oscillating Eclipsing Binary BG Peg

A. Liakos; P. Niarchos

doi:doi:10.1553/cia162s73

Michael BREGER (Ed.)

Communications in Asteroseismology Volume 162, 2011

Die Serie Communications in Asteroseismology (CoAst) stellt eine international gefragte Plattform für wissenschaftliche Publikationen der neuesten Forschungsergebnisse auf dem Gebiet der Asteroseismologie dar. Forschungsgegenstand der Asteroseismologie sind veränderliche und pulsierende Sterne. Neben den halbjährlich erscheinenden regulären Ausgaben mit Beiträgen aus der laufenden Forschung werden auch Sonderausgaben für Konferenzberichte bzw. Programmhandbücher herausgegeben.

Contents

Analyses of Crawfords uvby ß calibrations using the pulsational variations of FG Vir by P.Haas
A spectroscopic study of the hybrid pulsator γ Pegasi by C. P. Pandey, T.Morel, M. Briquet, et al.
Frequency analysis of five short periodic pulsators by A. Liakos, P.Niarchos
Update and Additional Frequencies for Kepler Star KIC 970032 by Joyce A. Guzik, Michel Breger
New pulsation analysis of the oscillating Eclipsing Binary BG Peg by A. Liakos, P.Niarchos

…

The publication series of Communications in Asteroseismology (CoAst) is one of the most important international journals in the field of asteroseismology. Asteroseismology is the science of variable and pulsating stars. Every six months CoAst publishes a newsletter with papers on ongoing research projects. Besides these regular issues, special issues such as conference proceedings or program manuals are published in this series.

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New pulsation analysis of the oscillating Eclipsing Binary BG Peg

A. Liakos,

P. Niarchos

Communications in Asteroseismology 162, pp. 73-80, 2011/07/22

doi: 10.1553/cia162s73

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doi:10.1553/cia162

doi:10.1553/cia162s73

Abstract

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 δ Sct type. Three pulsation frequencies were identified in that star.

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Michael BREGER (Ed.)

Communications in Asteroseismology Volume 162, 2011

New pulsation analysis of the oscillating Eclipsing Binary BG Peg

€ 9,99

Abstract