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Photometric Study of Variable Stars in the Open Cluster NGC 6866

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We report the discovery of 19 variable stars and two blue stragglers in the field of the open cluster NGC 6866. Three of the variable stars we classify as δ Sct, two as γ Dor, four as W UMa, two as ellipsoidal variables, and one as an eclipsing binary. Seven stars show irregular variability. Two of the pulsators, δ Sct star NGC 6866-29 and γ Dor star NGC 6866-21, are multiperiodic. From an analysis of proper motions, we conclude that the δ Sct stars, one of the γ Dor stars and both blue stragglers are very probable members of the cluster. The position on the color-magnitude diagram of seven other variables suggests that they also belong to the cluster. The eclipsing binary, which we discover to be a new high velocity star, and the seven irregular variables are non-members. We discuss in detail the age and metallicity of open clusters that host γ Dor stars and we show that none of these parameters is correlated with the number of γ Dor stars in cluster.
Czasopismo
Rocznik
Strony
193--211
Opis fizyczny
Bibliogr. 87 poz., rys., tab., wykr.
Twórcy
  • Astronomical Institute, University of Wrocław, ul. Kopernika 11, Wrocław, Poland
autor
  • Astronomical Institute, University of Wrocław, ul. Kopernika 11, Wrocław, Poland
  • Astronomical Institute, University of Wrocław, ul. Kopernika 11, Wrocław, Poland
autor
  • Astronomical Institute, University of Wrocław, ul. Kopernika 11, Wrocław, Poland
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Typ dokumentu
Bibliografia
Identyfikator YADDA
bwmeta1.element.baztech-8d82a47d-343f-426b-85a0-364dbd4236c0
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