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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: | Прамац |
Ректацензија: | 07h53m05.61s |
Deклинација: | -52°40'29.1" |
Apparent магнитуда: | 7.717 |
Даљина: | 297.619 parsecs |
Proper motion RA: | -0.3 |
Proper motion Dec: | 11.4 |
B-T magnitude: | 9.188 |
V-T magnitude: | 7.839 |
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