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Issue A&A
Volume 410, Number 3, November II 2003
Page(s) 879 - 885
Section Stellar clusters and associations
DOI http://dx.doi.org/10.1051/0004-6361:20031311



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, 2

1  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 $\delta$ Scuti stars and one as Algol-type eclipsing binary. Two stars are slow variables with ambiguous classification. From absolute $V(RI)_{\rm C}$ photometry we have estimated the main characteristics of the cluster: $m-M=11\fm0\pm0\fm5,\ E(V-I)=0\fm4\pm0\fm1,\ E(V-R)=0\fm08\pm0\fm06\
(E(B-V)=0\fm2\pm0\fm15)$ and $d=1.3\pm0.6$ 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 -- $\delta$ Sct

Offprint request: L. L. Kiss, laszlo@physics.usyd.edu.au

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