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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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Osservazione e dati astrometrici
| Costellazione: | Poppa |  
    | Ascensione retta: | 06h42m36.38s |  
    | Declinazione: | -33°37'55.2" |  
    | Magnitudine apparente: | 9.943 |  
    
    
    | Moto proprio RA: | -4.5 |  
    | Moto proprio Dec: | 6.8 |  
    | B-T magnitude: | 11.209 |  
    | V-T magnitude: | 10.048 |  
    
 
 
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