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Preliminary photometric study of a pulsating component in the eclipsing binary AB Per

Published online by Cambridge University Press:  12 April 2016

S.-L. Kim ,
S.-G. Kwon ,
D.J. Lee ,
C.-U. Lee ,
H. Jin  and
J.W. Lee
S.-L. Kim
Affiliation:
Korea Astronomy Observatory, Daejeon, 305-348, Korea
S.-G. Kwon
Affiliation:
Korea Astronomy Observatory, Daejeon, 305-348, Korea
D.J. Lee
Affiliation:
Korea Astronomy Observatory, Daejeon, 305-348, Korea
C.-U. Lee
Affiliation:
Korea Astronomy Observatory, Daejeon, 305-348, Korea
H. Jin
Affiliation:
Korea Astronomy Observatory, Daejeon, 305-348, Korea
J.W. Lee
Affiliation:
Department of Astronomy and Space Science, Chungbuk National University, Cheongju, 361-763, Korea

Abstract

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We present new photometric results of the Algol-type semidetached eclipsing binary AB Per which was recently discovered to have a Delta Scuti pulsating component.

Type
Part 6. Binary stars and pulsation
Information
International Astronomical Union Colloquium , Volume 193: Variable Stars in the Local Group , 2004 , pp. 399 - 402
Copyright
Copyright © Astronomical Society of the Pacific 2004

References

Kim, S.-L., Lee, J.W., Kwon, S.-G., Youn, J.-H., Mkrtichian, D., Kim, C. 2003, A&A, 405, 231 Google Scholar
Glazunova, L.V. 1999, Astronomy Letters, 25, 467 Google Scholar