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A&A 410, 879-885 (2003)
DOI: 10.1051/0004-6361:20031311
The first CCD photometric study of the open cluster NGC 2126
A. Gáspár1, 2, L. L. Kiss3, 2, T. R. Bedding3, A. Derekas3, 2, S. Kaspi4, Cs. Kiss5, K. Sárneczky6, 2, Gy. M. Szabó1 and M. Váradi1, 21 Department of Experimental Physics and Astronomical Observatory, University of Szeged, Szeged, Dóm Tér 9, 6720, Hungary
2 Guest Observer at Konkoly Observatory
3 School of Physics, University of Sydney 2006, Australia
4 School of Physics and Astronomy and the Wise Observatory, Tel-Aviv University, Tel-Aviv 69978, Israel
5 Konkoly Observatory of the Hungarian Academy of Sciences, PO Box 67, 1525 Budapest, Hungary
6 Astronomical Observatory, Szeged, Hungary
(Received 1 April 2003 / Accepted 18 August 2003 )
Abstract
We present the first CCD photometric observations of the northern
open cluster NGC 2126. Data were taken on eight nights in February and December
2002 with a total time span of ~57 hours. Almost 1000 individual
V-band
frames were examined to find short-period variable stars. We discovered six new
variable stars, of which one is a promising candidate for an
eclipsing binary with a pulsating component. Two stars were classified
as
Scuti stars and one as Algol-type eclipsing binary. Two stars are
slow variables with ambiguous classification. From absolute
photometry we
have estimated the main characteristics of the cluster:
and
kpc. Cluster membership
is suggested for three variable stars from their positions on the
colour-magnitude diagram.
Key words: open cluster and associations: general -- open clusters and associations: individual: NGC 2126 -- stars: variables: general --
Offprint request: L. L. Kiss, laszlo@physics.usyd.edu.au
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Tables at the CDS
© ESO 2003
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