Hyades and Sirius supercluster members brighter than magnitude(V) 7.1. I - The first six hours of right ascension

Details Hyades and Sirius supercluster members brighter than magnitude(V) 7.1. I - The first six hours of right ascension Hyades and Sirius supercluster members brighter than magnitude(V) 7.1. I - The first six hours of right ascension

Sep 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985pasp...97..807e&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 97, Sept. 1985, p. 807-823.

Astronomy and Astrophysics

Astronomy

15

Star Clusters, Stellar Magnitude, Stellar Motions, Astronomical Photometry, Radial Velocity, Stellar Luminosity, Tables (Data)

Scientific paper

This is the first of four papers listing the probable members of the Hyades and Sirius superclusters among stars brighter than V = 7.1 mag. The star sample is contained in the Bright Star Catalogue and its Supplement, augmented with a further supplement of 550 stars found during various observing programs over the past 40 years. Accurate, four-color and H-beta, or (RI), photometry is available for most of the supercluster members. The criteria for membership are the comparisons of the proper motion, radial velocity, and luminosity obtained from the supercluster parameters with the observed motions and the luminosity derived from the photometric parameters. New proper motions, based on all available catalogs, have been derived for the additional 550 stars discussed here, as well as for all supercluster members.

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