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Radial velocities in three fields along the southern galactic equator
A list of radial velocities for 764 stars is given for three fields inthe Vela-Carina region of the galaxy. They were obtained from GPO-platestaken at La Silla and reduced following Fehrenbach's method.Slit-spectra were collected with the 152 cm-spectrographic telescope atLa Silla, to derive an accurate radial velocity for a sufficient numberof calibration stars: out of the 29 stars, 26 had no formerly publishedvalue. The global motions of 10 to 14 km/s can be considered as normalon the basis of galactic rotation. Some stars, however, show highvelocities, and are therefore marked with one or two asterisks in thetable.
| Five-channel photometry of cepheids and supergiants in the southern Milky Way.
Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1976A&AS...24..413P&db_key=AST
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Datos observacionales y astrométricos
| Constelación: | Vela |
| Ascensión Recta: | 09h20m27.66s |
| Declinación: | -52°32'27.8" |
| Magnitud Aparente: | 8.583 |
| Distancia: | 10000000 parsecs |
| Movimiento Propio en Ascensión Recta: | -2.8 |
| Movimiento Propio en Declinación: | 3.4 |
| B-T magnitude: | 9.416 |
| V-T magnitude: | 8.652 |
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