The study of the rotation of the globular cluster 47 TUC

Details The study of the rotation of the globular cluster 47 TUC The study of the rotation of the globular cluster 47 TUC

Jan 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988pazh...14...31s&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 14, Jan. 1988, p. 31-36. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

1

Globular Clusters, Radial Velocity, Stellar Rotation, Astronomical Catalogs, Distance

Scientific paper

The rotation of 47 Tuc (NGC 104) was determined using the radial velocities of 159 stars listed in the catalogue of Major et al. (1983). The rotation parameters are functions of the distance from the center of the cluster. In the center the projection of the angular velocity is of the order of 10-5yr-1 and decreases rapidly with the distance.

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