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Photometry of astrometric reference stars
UBVRI, DDO, and uvby, H-beta photometry of astrometric reference starsis presented. Spectral types and luminosity classifications made fromthe colors are used to determine their spectroscopic parallaxes. In thispaper, colors for 309 stars in 25 regions are given, and classificationsfor 210 stars have been made. These stars form reference frames in theAllegheny Observatory Multichannel Astrometric Photometer astrometricprogram, and in the Praesepe cluster reduced by Russell (1976). It isfound that the present photometric spectral types are reliable to within2.5 spectral subclasses.
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Observation and Astrometry data
| Constellation: | かに座 |
| Right ascension: | 09h13m11.58s |
| Declination: | +14°44'49.8" |
| Apparent magnitude: | 9.359 |
| Proper motion RA: | 4.8 |
| Proper motion Dec: | -11.2 |
| B-T magnitude: | 9.533 |
| V-T magnitude: | 9.374 |
Catalogs and designations:
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