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Photometry of stars in the uvgr system
Photoelectric photometry is presented for over 400 stars using the uvgrsystem of Thuan and Gunn. Stars were selected to cover a wide range ofspectral type, luminosity class, and metallicity. A mean main sequenceis derived along with reddening curves and approximate transformationsto the UBVR system. The calibration of the standard-star sequence issignificantly improved.
| Colors, luminosities, and motions of the nearer G-type stars
Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1964AJ.....69..570E&db_key=AST
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Observation and Astrometry data
| Constellation: | ペガスス座 |
| Right ascension: | 22h54m35.65s |
| Declination: | +29°21'30.9" |
| Apparent magnitude: | 8.746 |
| Distance: | 129.87 parsecs |
| Proper motion RA: | 37.8 |
| Proper motion Dec: | 7.9 |
| B-T magnitude: | 9.349 |
| V-T magnitude: | 8.796 |
Catalogs and designations:
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