Observed radii and structural parameters of star clusters in the SMC. III

Details Observed radii and structural parameters of star clusters in the SMC. III Observed radii and structural parameters of star clusters in the SMC. III

Aug 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986a%26as...65..207k&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 65, no. 2, Aug. 1986, p. 207-232.

Astronomy and Astrophysics

Astrophysics

12

Astronomical Catalogs, Magellanic Clouds, Spatial Distribution, Star Clusters, Stellar Motions, Stellar Structure, Astronomical Photography, Mass Distribution, Milky Way Galaxy, Radii, Star Distribution

Scientific paper

The tidal radii, concentration parameters and masses of 24 star clusters in the SMC have been derived by means of star counts. In this investigation the seven most distant clusters (with projected distances from the rotation centre similar to the halo radius) are included as well and their masses were found to be about one hundred times lower than those of the halo clusters of our own Galaxy.

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