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2 Acta Astronomica

2 2006

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Eclipsing Binaries in the Open Cluster NGC 2243. II. Absolute Properties of NVCMa

Kaluzny J., Pych W., Rucinski S. M., Thompson I. B.

Acta Astronomica

2006

Vol. 56, No. 3

237--252

We present echelle spectroscopic data for five eclipsing binary stars and two giant stars in the field of the open cluster NGC 2243. The average cluster velocity is determined to be +60.4±0.6 km/s. Four of the eclipsing binaries are very likely members of the cluster based on their observed radial velocities. The absolute parameters of cluster member NV CMa are determined by analyzing photometric and radial velocity data. We obtain 1.089±0.010 Msolar and 1.221±0.031 Rsolar for the primary, and 1.069±0.010 Msolar and 1.178±0.037 Rsolar for the secondary. Both components of the binary are located on the Main Sequence, about 1 mag below the turn-off point on the cluster color-magnitude diagram. Using model age-luminosity and age-radius relations we obtain 4.35±0.25 Gyr for the age of NV CMa. The derived age is, however, very sensitive to the adopted metallicity of the cluster. We demonstrate that a meaningful determination of the ages of objects like NV CMa based on evolutionary models is possible only if their metallicity is known with a relative accuracy of a few percent. The distance moduli calculated for the components of NV CMa agree closely with each other, and imply an apparent distance modulus of the cluster of (m-M)V=13.24±0.08 mag.

Eclipsing Binaries in the Open Cluster NGC 2243 - I. Photometry

Kaluzny J., Krzeminski W., Thompson I. B., Stachowski G.

Acta Astronomica

2006

Vol. 56, No. 1

51--63

We obtained BV time series photometry for 12 variable stars from the field of the old open cluster NGC 2243. The sample includes 3 newly identified detached/semi-detached binaries. There are now four detached eclipsing binaries which are likely members of the cluster. Determination of the absolute parameters of the components would provide a valuable check on evolutionary models of low-mass stars. An accurate ephemeris and orbital period analysis are presented for the previously-known detached binary NV CMa. We also provide ephemerides for seven other periodic variables. We show that three contact binaries are likely members of the cluster.