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Hyades and Sirius supercluster members brighter than magnitude (V) 7.1. II - Right ascension six to twelve hours The present star sample is contained in the Bright Star Catalogue andits Supplement, augmented with a further supplement of 788 stars foundduring various observing programs over the past 40 years. Accurate,four-color and H-beta, or (RI), photometry is available for most of thesupercluster members. The criteria for membership are the comparisons ofthe proper motion, radial velocity, and luminosity obtained from thesupercluster parameters with the observed motions and the luminosityderived from the photometric parameters. New proper motions, based onall available catalogs, have been derived for the additional 788 starsdiscussed here, as well as all supercluster members.
| Catalog of Indidual Radial Velocities, 0h-12h, Measured by Astronomers of the Mount Wilson Observatory Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1970ApJS...19..387A&db_key=AST
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Membre dels grups següents:
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Dades d'Observació i Astrometria
Constel·lació: | Antlia |
Ascensió Recta: | 09h29m40.44s |
Declinació: | -26°35'39.3" |
Magnitud Aparent: | 6.543 |
Distancia: | 150.15 parsecs |
Moviment propi RA: | -84.8 |
Moviment propi Dec: | -31.7 |
B-T magnitude: | 7.69 |
V-T magnitude: | 6.638 |
Catàlegs i designacions:
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