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Hyades and Sirius supercluster members brighter than magnitude(V) 7.1. I - The first six hours of right ascension
This is the first of four papers listing the probable members of theHyades and Sirius superclusters among stars brighter than V = 7.1 mag.The star sample is contained in the Bright Star Catalogue and itsSupplement, augmented with a further supplement of 550 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 550 starsdiscussed here, as well as for all supercluster members.
| VI photometry of selected SAO stars
Johnson V- and I-band photoelectric photometry has been obtained for 158SAO stars in a continuing program in support of the Near InfraredPhotographic Sky Survey. These data are utilized in the calibration ofthe survey photographs and are presented here to assist other programsreliant upon access to photometry in the photographic infrared.
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Member of following groups:
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Observation and Astrometry data
| Constellation: | Orion |
| Right ascension: | 05h52m26.88s |
| Declination: | +06°12'33.9" |
| Apparent magnitude: | 6.911 |
| Distance: | 142.857 parsecs |
| Proper motion RA: | -8.4 |
| Proper motion Dec: | -18.4 |
| B-T magnitude: | 8.164 |
| V-T magnitude: | 7.015 |
Catalogs and designations:
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