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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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Observation and Astrometry data
| Constellation: | Vela |
| Right ascension: | 09h24m56.34s |
| Declination: | -53°24'38.9" |
| Apparent magnitude: | 9.396 |
| Proper motion RA: | -6.6 |
| Proper motion Dec: | 3.8 |
| B-T magnitude: | 9.443 |
| V-T magnitude: | 9.4 |
Catalogs and designations:
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INHABITED SKY
