Photoelectric photometry of star clusters in M31. IX

Details Photoelectric photometry of star clusters in M31. IX Photoelectric photometry of star clusters in M31. IX

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983pazh....9..393s&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 9, July-Aug. 1983, p. 393, 394) Soviet Astronomy Letters (ISSN 0360-0327), vol. 9, July

Astronomy and Astrophysics

Astronomy

1

Astronomical Photometry, Globular Clusters, Star Clusters, Ubv Spectra, Andromeda Galaxy, Electrophotometry

Scientific paper

A series of photoelectric UBV observations of globular clusters in the Andromeda Nebula (M31), conducted under a program that has been in progress since 1974, is presented. The observations were made on the night of October 15/16, 1982 at the Cassegrain focus of the 2.6-m Shain reflector of the Crimean Astrophysical Observatory. The observations raise the total number of globular clusters (or objects once thought to be globular clusters) in M31 and its companions from 344 to 351. Also, photometric parameters of several objects measured earlier have been refined. It is estimated that about a hundred probable clusters, faint objects located chiefly in the central region of M31, still lack photoelectric data.

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