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CCD Photometry of Variable Stars in the Galactic Open Cluster NGC 7419

Published online by Cambridge University Press:  12 April 2016

Z. Kołaczkowski ,
A. Pigulski  and
G. Kopacki
Z. Kołaczkowski
Affiliation:
Wrocław University Observatory, Kopernika 11, 51-622 Wrocław, Poland
A. Pigulski
Affiliation:
Wrocław University Observatory, Kopernika 11, 51-622 Wrocław, Poland
G. Kopacki
Affiliation:
Wrocław University Observatory, Kopernika 11, 51-622 Wrocław, Poland

Abstract

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We present results of a CCD variability search in the field of the young open cluster NGC 7419. This cluster contains a large number of Be stars and almost all of them turned out to be variable. They show mostly irregular variations on different time-scales with ranges up to 0.4 mag in the IC band. The most interesting result is the discovery of short-period variability in some of the Be stars.

Type
Part 1.4. Pulsating Stars in Clusters
Information
International Astronomical Union Colloquium , Volume 185: Radial and Nonradial Pulsations as Probes of Stellar Physics , 2002 , pp. 150 - 151
Copyright
Copyright © Astronomical Society of the Pacific 2002

References

Balona, L.A. & Rozowsky, J. 1991, MNRAS, 251, 66 CrossRefGoogle Scholar
Beauchamp, A., Moffat, A.F.J., & Drissen, L. 1994, ApJS, 93, 187 CrossRefGoogle Scholar
Bhatt, B.C., Pandey, A.K., Mohan, V., Mahra, H.S., & Paliwal, D.C, 1993, Bull. Astron. Soc. India, 21, 33 Google Scholar
Pigulski, A. & Kopacki, G., 2000, A&AS, 146, 465 Google Scholar
Stetson, P.B. 1987, PASP, 99, 191 CrossRefGoogle Scholar