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Eclipse Mapping of Non-Radial Pulsation in Binary Stars

Published online by Cambridge University Press:  12 April 2016

J. Nuspl  and
I.B. Bíró
J. Nuspl
Affiliation:
Konkoly Observatory, Budapest, Hungary
I.B. Bíró
Affiliation:
Baja Astronomical Observatory, Baja, Hungary

Abstract

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We review a slightly modified method of eclipse mapping, applicable to mode identification in eclipsing binaries containing a pulsating component. The observed light curve is used by the procedure without removing from it the badly determined eclipsing part.

Type
Part 1.2. Pulsations in Close Binaries
Information
International Astronomical Union Colloquium , Volume 185: Radial and Nonradial Pulsations as Probes of Stellar Physics , 2002 , pp. 100 - 101
Copyright
Copyright © Astronomical Society of the Pacific 2002

References

Horne, K. 1985, MNRAS, 213, 129 CrossRefGoogle Scholar
Kallrath, J.& Milone, E.F. 1999, Eclipsing Binary Stars, (Springer Verlag)Google Scholar
Ohshima, O., Narusawa, S., Akazawa, H., et al. 2001, AJ, 122, 418 Google Scholar
Rodríguez, E., Claret, A., Sedano, J.L., et al. 1998, A&A, 340, 196 Google Scholar