UBV photometry in the cluster NGC 7510 (Barbon+, 1996)

Details UBV photometry in the cluster NGC 7510 (Barbon+, 1996) UBV photometry in the cluster NGC 7510 (Barbon+, 1996)

Sep 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ycat..41150325b&link_type=abstract

VizieR On-line Data Catalog: J/A+AS/115/325. Originally published in: 1996A&AS..115..325B

Physics

Clusters: Open, Photometry: Ubv

Scientific paper

Three-colour photographic photometry of the young open cluster NGC 7510 based upon UBV observations made with the 122cm and 182cm Asiago reflectors is presented here. A mean colour excess E(B-V)=1.12, a distance of 3.09kpc could be achieved for this cluster and 31 stars could be identified as photometric physical members. An age of 107years has been derived by comparison with standard isochrones. The discrepancy between the photometric and spectroscopic distances obtained for some stars is discussed and comparisons with recent investigations of the same object are also given. (1 data file).

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