Physics
Scientific paper
Jun 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990kfnt....6...14m&link_type=abstract
Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 6, May-June 1990, p. 14-17, 40. In Russian.
Physics
Main Sequence Stars, Peculiar Stars, Stellar Motions, Density Distribution, Stellar Evolution, Stellar Spectra
Scientific paper
The differences in the proper motions of chemically peculiar and
main-sequence stars are determined. It is found that the mean values and
dispersions of proper motions for the chemically peculiar stars are
lower than those of the main-sequence stars.
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