Hostname: page-component-586b7cd67f-rcrh6 Total loading time: 0 Render date: 2024-11-26T13:52:31.643Z Has data issue: false hasContentIssue false

Eclipse Mapping of Non-Radial Pulsation in Binary Stars

Published online by Cambridge University Press:  12 April 2016

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

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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
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