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DDO Observations of Southern Stars
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| The K-giant population at the South Galactic Pole
CN anomalies and distances from the galactic plane have been derivedthrough DDO photometry for 171 late-type giant and subgiant stars nearthe South Galactic Pole. The previously found trend of the difference inCN concentration with distance (approximately equal to 0.09/kpc) holdsto approximately 2 kpc, but at greater distances from the plane theslope becomes approximately zero. The giants beyond 2 kpc are ofessentially normal composition or only slightly underabundant in heavierelements.
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Membre dels grups següents:
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Dades d'Observació i Astrometria
| Constel·lació: | 조각가자리 |
| Ascensió Recta: | 00h59m55.38s |
| Declinació: | -31°16'15.1" |
| Magnitud Aparent: | 9.235 |
| Moviment propi RA: | 78.1 |
| Moviment propi Dec: | 6.2 |
| B-T magnitude: | 10.17 |
| V-T magnitude: | 9.313 |
Catàlegs i designacions:
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