摘要：AbstractHere we have obtained theBVRI CCDphotometry down to a limiting magnitude ofV∼20for the southern poorly studied open cluster NGC 6631. It is observed from the 1.88m Telescope of Kottamia Observatory in Egypt. About 3300 stars have been observed in an area of∼10′×10′around the cluster center. The main photometric parameters have been estimated and compared with the results that determined for the cluster usingJHKs 2MASSphotometric database. The cluster’s diameter is estimated to be 10arcmin; the reddeningE(B-V)=0.68±0.10mag,E(J-H)=0.21±0.10mag, the true modulus(m-M)o=12.16±0.10mag, which corresponds to a distance of 2700±125pc and age of 500±50Myr.
关键词：KeywordsGalaxy: open clusters and associationsIndividual: NGC 6631AstrometryStars: luminosity functionMass function
