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Submit a new article| Radial velocities of faint stars from objective prism plates A simple method by which the approximate radial velocity of a star maybe obtained from objective prism plates is described in detail. Themethod has been used to derive the velocities of 41 faint stars, most ofwhich have metal-weak spectra and are shown to be high-velocity objects.It is shown that this method may be generalized so that the radialvelocities for all measurable stars on an objective prism plate can beobtained.
 
 
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 Observation and Astrometry data
| Constellation: | Corbeau |  | Right ascension: | 12h01m23.29s |  | Declination: | -20°39'49.8" |  | Apparent magnitude: | 7.561 |  | Distance: | 354.61 parsecs |  | Proper motion RA: | -23.2 |  | Proper motion Dec: | -36.4 |  | B-T magnitude: | 8.908 |  | V-T magnitude: | 7.673 |  Catalogs and designations:
 
 
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