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First radial velocities for 146 bright F- and G-type stars We have obtained an average of 5.7 radial velocities for 146 northernstars of types F and G (all luminosity classes) listed in 'A Supplementto the Bright Star Catalogue' as having no previously known radialvelocity measures. Those were obtained with charge coupled devices(CCDs) and a cross-correlation technique; the intrinsic velocityaccuracy, based on stars of apparently constant velocity, is probablyless than +/- 0.3 km/s per mean. Of those stars 14% are newly discoveredSB2 stars. The prevelance of rapid profile variations (in minutes orhours) in most of the broad-lined F-type stars makes it difficult toobtain accurate measures for them.
| UvbyH-beta photoelectric and CCD photometry of IC 4651 An analysis of uvbyH-beta photoelectric and CCD photometry of IC4651shows a Fe/H abundance ratio of 0.23 + or - 0.02, an E(b-y) value of0.064 + or - 0.006, and an age on the system of VandenBerg (1985) of 2.4+ or - 0.2 x 10 to the 9th yr. Scatter noted in the clustercolor-magnitude diagram can be explained by binaries, nonmembers, and ablueward hook due to the hydrogen-exhaustion phase. The cluster turnoffindicates some evidence for the presence of bimodality which issuggested to be the result of nonstandard evolution near theBohm-Vitense gap.
| MK classifications for F-and G-type stars. 3. Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1974AJ.....79..682H&db_key=AST
| Lichtelektrische UBV-Photometrie von Standardsternen und in vier Sternfeldern am Äquator Not Available
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Datos observacionales y astrométricos
Constelación: | Acuario |
Ascensión Recta: | 20h46m01.21s |
Declinación: | -00°20'25.5" |
Magnitud Aparente: | 6.769 |
Distancia: | 200 parsecs |
Movimiento Propio en Ascensión Recta: | 3.7 |
Movimiento Propio en Declinación: | -6.7 |
B-T magnitude: | 7.97 |
V-T magnitude: | 6.869 |
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