Variable stars in the Open Cluster M11 (NGC 6705) J.-R. Koo Department of Astronomy and Space Science, Chungnam National University, Daejeon 305-764, Korea; and Korea Astronomy and Space Science Institute, Daejeon 305-348, Korea
[email protected] S.-L. Kim Korea Astronomy and Space Science Institute, Daejeon 305-348, Korea
[email protected] S.-C. Rey Department of Astronomy and Space Science, Chungnam National University, Daejeon 305-764, Korea C.-U. Lee Korea Astronomy and Space Science Institute, Daejeon 305-348, Korea Y. H. Kim Department of Astronomy and Space Science, Chungnam National University, Daejeon 305-764, Korea Y. B. Kang Department of Astronomy and Space Science, Chungnam National University, Daejeon 305-764, Korea; and Korea Astronomy and Space Science Institute, arXiv:0709.1180v1 [astro-ph] 8 Sep 2007 Daejeon 305-348, Korea and Y.-B. Jeon Korea Astronomy and Space Science Institute, Daejeon 305-348, Korea ABSTRACT V -band time-series CCD photometric observations of the intermediate-age open clus- ter M11 were performed to search for variable stars. Using these time-series data, we – 2 – carefully examined light variations of all stars in the observing field. A total of 82 vari- able stars were discovered, of which 39 stars had been detected recently by Hargis et al. (2005). On the basis of observational properties such as variable period, light curve shape, and position on a color-magnitude diagram, we classified their variable types as 11 δ Scuti–type pulsating stars, 2 γ Doradus–type pulsating stars, 40 W UMa–type contact eclipsing binaries, 13 Algol–type detached eclipsing binaries, and 16 eclipsing binaries with long period.