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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.
 
  |  Six UBV photoelectric sequences in VELA (l=257 degres to 281 degres.). Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1975A&AS...19...45D&db_key=AST
 
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Dades d'Observació i Astrometria
| Constel·lació: | Vela |  
    | Ascensió Recta: | 09h23m05.33s |  
    | Declinació: | -51°54'15.2" |  
    | Magnitud Aparent: | 8.823 |  
    
        | Distancia: | 411.523 parsecs |  
        
    
    | Moviment propi RA: | -13.7 |  
    | Moviment propi Dec: | 11.9 |  
    | B-T magnitude: | 8.888 |  
    | V-T magnitude: | 8.829 |  
    
 
 
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