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Southern metal-poor stars - UBVRI photometry Considering the study of subdwarf kinematics and metallicities by Eggen,Lynden-Bell, and Sandage (1962), UBVRI photometry and normalizedultraviolet excesses are presented for 178 metal-poor stars, 144 ofwhich are contained in the kinematically unbiased list of Bidelman andMacConnell (1973). The Lowell 0.6 m telescope at Cerro Tololo was used,equipped with a single-channel photometer and a Ga-As photomultiplier.The final magnitudes and colors, number of observations, value ofdelta(U-B)0.6 (if B-V lies between 0.35 and 0.90), B and M class, andpublished spectral types for these stars are presented; severalextremely metal-poor stars are evident. In addition, sixteen nearbyvisual companions of the stars were measured, and their magnitudes andcolors are given.
 
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Datos observacionales y astrométricos
| Constelación: | Vela |  
    | Ascensión Recta: | 10h45m00.65s |  
    | Declinación: | -43°51'58.8" |  
    | Magnitud Aparente: | 8.856 |  
    
        | Distancia: | 309.598 parsecs |  
        
    
    | Movimiento Propio en Ascensión Recta: | -19.1 |  
    | Movimiento Propio en Declinación: | 8.1 |  
    | B-T magnitude: | 9.12 |  
    | V-T magnitude: | 8.878 |  
    
 
 
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