Astronomy and Astrophysics – Astronomy
Scientific paper
Nov 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986mnras.223..183i&link_type=abstract
Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 223, Nov. 1, 1986, p. 183-188. Research supported by Mo
Astronomy and Astrophysics
Astronomy
69
Chromosphere, Pre-Main Sequence Stars, Star Clusters, Stellar Evolution, Stellar Rotation, K Stars, Pleiades Cluster, Stellar Activity, Stellar Motions
Scientific paper
The space velocities U, V, W, for the rapidly rotating late-type stars AB Dor (HD 36705) and PZ Tel (HD 174429) are shown to be identical within the observational uncertainties with those of the Pleiades moving group (Local Association). The authors suggest that these two stars are members of this group, and hence stars in the final stages of their approach to the main sequence. The authors believe that AB Dor and PZ Tel are very similar to the recently discovered rapidly rotating Pleiades cluster K dwarfs.
Coates D. W.
Innis John L.
Thompson Kevin
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