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Uvbyβ photometry of all stars earlier than G0 and brighter than m_pg_~10.3mag in Selected Area 194 Four-colour and Hβ photometry is introduced for 594 stars earlierthan G0 in the Kapteyn's Selected Area 194. The results give V, b-y,m_1_, c_1_, and β on the standard systems, with overall rms errorsfor one observation of one star of 0.009mag, 0.004mag, 0.006mag,0.009mag, and 0.009mag, respectively. The data cover an area of about5deg x 5deg and is intended for an investigation of the distribution ofthe interstellar medium toward the northern part of the SouthernCoalsack and its surroundings. A comparison to earlier results obtainedby other authors has shown that the c_1_ indices obtained for the latetype stars were underestimated, in average, by 0.020mag. Since suchdifference may account for an error of little more than 10% in theestimated stellar distances, a correction was applied to the c_1_ indexof these stars.
 
  |  Walraven photometry of nearby southern OB associations Homogeneous Walraven (VBLUW) photometry is presented for 5260 stars inthe regions of five nearby southern OB associations: Scorpio Centaurus(Sco OB2), Orion OB1, Canis Major OB1, Monoceros OB1, and Scutum OB2.Derived V and (B - V) in the Johnson system are included.
 
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 Membre dels grups següents:
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Dades d'Observació i Astrometria
| Constel·lació: | Centaurus |  
    | Ascensió Recta: | 13h09m28.79s |  
    | Declinació: | -58°44'31.6" |  
    | Magnitud Aparent: | 9.006 |  
    
        | Distancia: | 724.638 parsecs |  
        
    
    | Moviment propi RA: | -6.5 |  
    | Moviment propi Dec: | -0.5 |  
    | B-T magnitude: | 10.15 |  
    | V-T magnitude: | 9.101 |  
    
 
 
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