• Michael BREGER (Ed.)

Communications in Asteroseismology Volume 162, 2011

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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 Crawford’s 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.



Verlag der Österreichischen Akademie der Wissenschaften
Austrian Academy of Sciences Press
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Tel. +43-1-515 81/DW 3420, Fax +43-1-515 81/DW 3400
https://verlag.oeaw.ac.at, e-mail: verlag@oeaw.ac.at

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Communications in Asteroseismology Volume 162, 2011


ISBN 978-3-7001-7154-6
Print Edition
ISBN 978-3-7001-7223-9
Online Edition



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Verlag der Österreichischen Akademie der Wissenschaften
Austrian Academy of Sciences Press
A-1011 Wien, Dr. Ignaz Seipel-Platz 2,
Tel. +43-1-515 81/DW 3420, Fax +43-1-515 81/DW 3400
https://verlag.oeaw.ac.at, e-mail: bestellung.verlag@oeaw.ac.at
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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.

Published Online: 2011/07/22 12:35:00

Object Identifier: 0xc1aa5572 0x0029e6e8

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