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Photometry of Southern Hemisphere red dwarf stars
Results are presented for a photometric investigation of aspectroscopically selected sample of red dwarf stars in the SouthernHemisphere. Absolute magnitudes and distances for the stars areestimated from broadband red colors. Three stars which may besubluminous are identified, as are several stars which may be within 25pc. The tangential velocity and velocity dispersion of the sample aresimilar to values found in other studies of nearby late-type stars.
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Osservazione e dati astrometrici
| Costellazione: | Fenice |
| Ascensione retta: | 00h41m15.20s |
| Declinazione: | -52°19'01.9" |
| Magnitudine apparente: | 10.754 |
| Distanza: | 43.573 parsec |
| Moto proprio RA: | 0 |
| Moto proprio Dec: | 0 |
| B-T magnitude: | 12.437 |
| V-T magnitude: | 10.893 |
Cataloghi e designazioni:
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INHABITED SKY
