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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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| Сазвежђа: | Кентаур |  
    | Ректацензија: | 11h28m28.48s |  
    | Deклинација: | -55°53'14.5" |  
    | Apparent магнитуда: | 9.164 |  
    
    
    | Proper motion RA: | -53.7 |  
    | Proper motion Dec: | 18.3 |  
    | B-T magnitude: | 9.717 |  
    | V-T magnitude: | 9.21 |  
    
 
 
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