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Some New Possible Variable Stars II.
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| Preliminary UVBY calibrations for G and K type dwarf stars
Four-color uvby photometry for several hundred late-type dwarf stars oftypes G, K and M is discussed. Mean values of photometric indices aregiven for MK spectral types between F8/G0V and M2V. Preliminary standardrelations between the four-color indices are derived. Based onparallaxes and results from high-dispersion spectroscopic analyses,calibrations of the observed indices in terms of Mv, log Te and Fe/Hhave been derived. The means errors are 0.29 mag, 0.009 dex, and 0.17dex, respectively. The calibrations are valid for class-V stars of allpopulations between G0 and M2. If extreme population-II dwarfs areexcluded, the mean error of the abundance calibration decreases to 0.13dex. Calibrations in terms of log g have been attempted,, but the lowaccuracy of the spectroscopic g determinations does not inspireconfidence in the results. The possible contribution of a'fourth-parameter' variation to the mean errors of the calibrations isbriefly discussed. This fourth parameter could be the intrinsic heliumabundance of the stars.
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| Takýmyýldýz: | Pupa |
| Sað Açýklýk: | 06h32m36.62s |
| Yükselim: | -44°13'15.2" |
| Görünürdeki Parlaklýk: | 7.295 |
| Uzaklýk: | 100.1 parsek |
| özdevim Sað Açýklýk: | -1.2 |
| özdevim Yükselim: | -5.4 |
| B-T magnitude: | 7.559 |
| V-T magnitude: | 7.317 |
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