Photometric Study of Variable Stars in the Open Cluster NGC 6866

被引:0
|
作者
Molenda-Zakowicz, J. [1 ]
Kopacki, G. [1 ]
Steslicki, M. [1 ]
Narwid, A. [1 ]
机构
[1] Univ Wroclaw, Astron Inst, PL-50138 Wroclaw, Poland
来源
ACTA ASTRONOMICA | 2009年 / 59卷 / 02期
关键词
Stars: oscillations; Stars: variables: general; delta Sct; open clusters and associations: individual: NGC 6866; HIGH-RESOLUTION SPECTROSCOPY; TRANSITING EXTRASOLAR PLANETS; OLD OPEN CLUSTERS; PERSEI OPEN CLUSTER; GALACTIC DISK; STELLAR-SYSTEMS; METALLICITY DISTRIBUTION; CHEMICAL-COMPOSITION; ABUNDANCE GRADIENT; RADIAL-VELOCITIES;
D O I
暂无
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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 8 Set, two as gamma Dor, four as W UMa, two as ellipsoidal variables, and one as an eclipsing binary. Seven stars show irregular variability. Two of the pulsators, delta Set star NGC 6866-29 and gamma Dor star NGC 6866-21, are multiperiodic. From an analysis of proper motions, we conclude that the 8 Set stars, one of the gamma 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 gamma Dor stars and we show that none of these parameters is correlated with the number of gamma Dor stars ill cluster.
引用
收藏
页码:193 / 211
页数:19
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