On the membership of the outlying LMC clusters from radial velocities

Details On the membership of the outlying LMC clusters from radial velocities On the membership of the outlying LMC clusters from radial velocities

May 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981aj.....86..667c&link_type=abstract

Astronomical Journal, vol. 86, May 1981, p. 667, 668.

Astronomy and Astrophysics

Astronomy

15

Giant Stars, Globular Clusters, Magellanic Clouds, Radial Velocity, Stellar Motions, Astrometry, Distance, Stellar Spectrophotometry, Tides

Scientific paper

New radial velocity data have been obtained for several giant stars in
the LMC globular clusters NGC 1466, 1841, and 2257. This information,
together with a rediscussion of the clusters' true distances from the
center of the Large Cloud, suggests that NGC 1466 may belong to the
Galaxy rather than to the LMC.

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