摘要
本文给出了疏散星团NGC2286天区中305颗恒星的照相B、V星等,结合其它资料得到了星团的平均色余值为E_(B-V)=0.40m±0.07m,距离模数10.90m±0.10m,相应的距离为r 1510pc±70pc,年龄估值为6×10~7年,由得到的星团HR图讨论了星团的其它性质。
Photographic V magnitudes and (B - V) colours in the UBV system are determined for 305 stars in the field of the open cluster NGC 2286, and the rms errors of V and (B - V) for one plate are estimated to be σv = 0.m063, and σB-v = 0.m084, respectively. The reddening value of the cluster is 0.m40±0.m07. The derived distance modulus to the cluster is approximately 10.m9±0.m1. Using the composite diagram method, the age of the cluster is estimated as 6 × 107 yr. The HR diagram of the cluster is obtained and discussed. Furthermore, a better determination of membership of the cluster is made based on the proper motion membership probabilities and the photometric data of these 305 stars.
基金
国家自然科学基金
关键词
恒星
银河星团
照相
测光
HR图
Stars-Open cluster-Photographic Photometry-HR diagram