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Empirical Calibration of Absolute Magnitudes for G-K Dwarfs and Subdwarfs in the Vilnius Photometric System Calibrations giving l M_V as functions of [Fe/H] and various intrinsiccolor indices of the Vilnius photometric system are derived for G--Kdwarfs and subdwarfs. The calibrations are based only on the stars withknown trigonometric parallaxes and allow one to estimate the absolutemagnitudes with a standard deviation of +/- 0.6 mag. Comparisons of ourcalibrations with the absolute magnitude estimates in the literatureshow a satisfactory agreement.
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Observation and Astrometry data
Constellation: | うみへび座 |
Right ascension: | 12h31m08.25s |
Declination: | -31°38'08.3" |
Apparent magnitude: | 7.888 |
Distance: | 98.717 parsecs |
Proper motion RA: | -48.9 |
Proper motion Dec: | -7.8 |
B-T magnitude: | 8.199 |
V-T magnitude: | 7.914 |
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