UBV three-colour photometric parameters of four galactic clusters near Cassiopeia

Details UBV three-colour photometric parameters of four galactic clusters near Cassiopeia UBV three-colour photometric parameters of four galactic clusters near Cassiopeia

Jan 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985a%26as...59...83f&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 59, Jan. 1985, p. 83-86. Research supported by the Swiss Nat

Astronomy and Astrophysics

Astrophysics

7

Astronomical Photometry, Galactic Structure, Star Clusters, Astronomical Photography, Cassiopeia Constellation, Ubv Spectra

Scientific paper

Becker's (1963) method A is the basis of the present determination of interstellar reddening and absorption, distance, earliest spectral type, and probable physical membership, for the four galactic clusters NGC 7510, Ba 2, Ba 3, and NGC 7654, near Cassiopeia. Photographic UBV measurements were obtained with the Asiago 65-cm Schmidt telescope in 1972. The coordinates of the clusters and their parameters are presented in tabular form.

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