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Rotational Velocities of Late-Type Stars
A calibration based on the results of Gray has been used to determineprojected rotational velocities for 133 bright stars with spectral typesof F, G, or K, most of which appear in {\it The Bright Star Catalogue}.The vast majority have {\it v} sin {\it i} $\leq$ 10 km s$^{-1}$ and,thus, are slow rotators. With the new calibration, projected rotationalvelocities have been determined for a sample of 111 late-type stars,most of which are chromospherically active. Some of the stars have hadtheir rotational velocities measured for the first time. (SECTION:Stars)
| Radial velocities of southern stars obtained with the photoelectric scanner CORAVEL. III - 790 late-type bright stars
Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1985A&AS...59...15A&db_key=AST
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| Сазвежђа: | Паун |
| Ректацензија: | 18h09m57.60s |
| Deклинација: | -59°02'24.0" |
| Apparent магнитуда: | 6.38 |
| Даљина: | 196.85 parsecs |
| Proper motion RA: | -24.8 |
| Proper motion Dec: | -3.6 |
| B-T magnitude: | 8.426 |
| V-T magnitude: | 6.559 |
Каталог и designations:
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INHABITED SKY
