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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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Membre dels grups següents:
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Dades d'Observació i Astrometria
| Constel·lació: | Corvus |
| Ascensió Recta: | 11h57m51.16s |
| Declinació: | -18°06'07.6" |
| Magnitud Aparent: | 8.555 |
| Distancia: | 137.741 parsecs |
| Moviment propi RA: | 4 |
| Moviment propi Dec: | -31.7 |
| B-T magnitude: | 9.14 |
| V-T magnitude: | 8.604 |
Catàlegs i designacions:
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NEWS@SKY (Science&Space News)
