Chemically peculiar and main-sequence stars - Distribution with respect to the Galactic z-coordinate

Details Chemically peculiar and main-sequence stars - Distribution with respect to the Galactic z-coordinate Chemically peculiar and main-sequence stars - Distribution with respect to the Galactic z-coordinate

Oct 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991kfnt....7...87m&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 7, Sept.-Oct. 1991, p. 87-92. In Russian.

Computer Science

Main Sequence Stars, Peculiar Stars, Star Clusters, Star Distribution, Stellar Composition, Galactic Structure, Spatial Distribution, Stellar Spectra

Scientific paper

The distribution of chemically peculiar (CP) and main-sequence (MS) stars with respect to the Galactic z-coordinate are obtained for three samples. A cluster analysis of the spatial distribution of the CP and MS stars shows that chemically peculiar stars in the direction of the Galactic anticenter tend to form compact space clusters, as was previously established for the nearest CP stars. The spatial distribution of MS stars is found to be more homogeneous.

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