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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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Gözlemler ve gökölçümü verileri
| Takýmyýldýz: | Kupa |
| Sað Açýklýk: | 11h53m38.14s |
| Yükselim: | -20°21'12.0" |
| Görünürdeki Parlaklýk: | 9.252 |
| özdevim Sað Açýklýk: | -26.7 |
| özdevim Yükselim: | 16.6 |
| B-T magnitude: | 9.896 |
| V-T magnitude: | 9.306 |
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