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Variable stars in the field of the young open cluster Roslund 2

Published online by Cambridge University Press:  18 February 2014

P. Sowicka
Affiliation:
Astronomical Observatory, Jagiellonian University, Orla 171, 30-244 Kraków, Poland, email: paula@byk.oa.uj.edu.pl
G. Handler
Affiliation:
Nicolaus Copernicus Astronomical Center, Bartycka 18, 00-716 Warsaw, Poland
R. Taubner
Affiliation:
Institut für Astronomie, Universität Wien, Türkenschanzstrasse 17, 1180 Wien, Austria
M. Brunner
Affiliation:
Institut für Astronomie, Universität Wien, Türkenschanzstrasse 17, 1180 Wien, Austria
V.-M. Passegger
Affiliation:
Institut für Astronomie, Universität Wien, Türkenschanzstrasse 17, 1180 Wien, Austria
F. Bauer
Affiliation:
Institut für Astronomie, Universität Wien, Türkenschanzstrasse 17, 1180 Wien, Austria
E. Paunzen
Affiliation:
Department of Theoretical Physics and Astrophysics, Masaryk University, Kotlarska 2, 611 37 Brno, Czech Republic
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Abstract

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The study of variable stars in open clusters via asteroseismology is a powerful tool for the study of stellar evolution and stars in general. That is because stars in clusters can be assumed to originate from the same interstellar cloud, so they share similar properties such as age and overall metallicity. We performed a search for variable stars in the field of the young open star cluster Roslund 2, with photoelectric and CCD photometry acquired at two different telescopes. Within the resulting light curves we have found 12 variable stars. Our measurements confirm three previously known variables.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2014 

References

Roslund, C. 1960, PASP, 72, 205Google Scholar
Kharchenko, N. V., Piskunov, A. E., Röser, S., Schilbach, E., & Scholz, R.-D. 2005, A&A, 438, 1163Google Scholar