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Red giants in open clusters. VIII. NGC 752
The results of an 18-year radial-velocity survey of 30 red giants in thefield of the open cluster NGC 752 are presented. The membership of 15stars is confirmed. Four spectroscopic binaries have been discoveredamong the members and three orbits have been determined for H75, 110 and208, with periods of 3321, 127 and 5276 days respectively. The binaryfrequency (27%) is normal. A search for additional members in a widesurrounding area (2degr ) yielded two possible new members: both areclump red giant candidates. The red giant distribution in thecolour-magnitude diagram is somewhat unusual, with a clump containing 8stars and a second, fainter feature extending to the blue, defined by 3or 4 stars, which is not accounted for by theoretical isochrones. Basedon observations collected at the Haute-Provence Observatory (France)
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Membre dels grups següents:
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Dades d'Observació i Astrometria
| Constel·lació: | Andromeda |
| Ascensió Recta: | 02h00m56.39s |
| Declinació: | +38°41'02.8" |
| Magnitud Aparent: | 8.243 |
| Distancia: | 371.747 parsecs |
| Moviment propi RA: | -5.7 |
| Moviment propi Dec: | -17.4 |
| B-T magnitude: | 10.041 |
| V-T magnitude: | 8.392 |
Catàlegs i designacions:
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INHABITED SKY
