Studies of nearby poor clusters - A3574 and S753

Details Studies of nearby poor clusters - A3574 and S753 Studies of nearby poor clusters - A3574 and S753

Jan 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991aj....101...57w&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 101, Jan. 1991, p. 57-65.

Astronomy and Astrophysics

Astronomy

41

Astronomical Photometry, Galactic Clusters, Astronomical Photography, Astronomical Spectroscopy, Galactic Rotation, Luminosity, Southern Sky

Scientific paper

Photometric and spectroscopic data are presented for two clusters, A3574 and S753, belonging to the Centaurus concentration of galaxies. The masses of the clusters are estimated at 1.5 x 10 to the 14th solar masses; no evidence of substructure has been detected in either cluster. The solution of a two-body linear orbit suggests that the clusters do not form a bound system, although the result is marginal.

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