Systematic search for members of the Hyades Supercluster. VI - The lower main sequence

Details Systematic search for members of the Hyades Supercluster. VI - The lower main sequence Systematic search for members of the Hyades Supercluster. VI - The lower main sequence

Jan 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985aj.....90...74e&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 90, Jan. 1985, p. 74-79.

Astronomy and Astrophysics

Astronomy

26

Dwarf Stars, Main Sequence Stars, Star Clusters, Star Distribution, Stellar Magnitude, Stellar Motions, Radial Velocity, Red Dwarf Stars, Stellar Parallax

Scientific paper

From a complete sample of stars with visual magnitude brighter than 15 and annual proper motion larger than 0.5 arcsec, 50 members of the Hyades Supercluster have been identified by their proper motion. The resulting main sequence is represented, for Mbol > +5.5 mag, by Mbol = 4.51+4.31(R-I) with a dispersion of 0.15 mag. The supercluster stars may represent 15% of the star density near the Sun. Two incomplete samples of red dwarfs, formed by Vyssotsky and by Weis, are also examined for supercluster stars and add 34 members.

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