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The VELA star cloud. III - The B8 to A0 stars and interstellar reddening The present discussion of intermediate band and H-beta observations of360 HD stars B8-A0 in Vela, and all of the CPD stars in a small adjacentregion, notes that the interstellar absorption in both cases can beunderstood as a combination of three absorbing clouds of 1 kpc-A(V) =1.5, 0.5, and 0.17. The major difference in the two environments is thepresence of numerous T Tauri stars in Taurus. Several clusters in theVela region are discussed.
 
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Observation and Astrometry data
| Constellation: | ほ座 |  
    | Right ascension: | 08h15m37.53s |  
    | Declination: | -49°59'34.5" |  
    | Apparent magnitude: | 7.568 |  
    
        | Distance: | 609.756 parsecs |  
        
    
    | Proper motion RA: | -3.9 |  
    | Proper motion Dec: | 3.5 |  
    | B-T magnitude: | 7.56 |  
    | V-T magnitude: | 7.568 |  
    
 
 
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