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Research Note Hipparcos photometry: The least variable stars
The data known as the Hipparcos Photometry obtained with the Hipparcossatellite have been investigated to find those stars which are leastvariable. Such stars are excellent candidates to serve as standards forphotometric systems. Their spectral types suggest in which parts of theHR diagrams stars are most constant. In some cases these values stronglyindicate that previous ground based studies claiming photometricvariability are incorrect or that the level of stellar activity haschanged. Table 2 is only available in electronic form at the CDS viaanonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or viahttp://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/A+A/367/297
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Member of following groups:
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Observation and Astrometry data
| Constellation: | Baleine |
| Right ascension: | 01h34m51.32s |
| Declination: | -03°31'26.0" |
| Apparent magnitude: | 6.437 |
| Distance: | 251.256 parsecs |
| Proper motion RA: | 12.4 |
| Proper motion Dec: | -33.1 |
| B-T magnitude: | 8.207 |
| V-T magnitude: | 6.584 |
Catalogs and designations:
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