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HD 80866


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The chemical evolution of the solar neighborhood. I - A bias-free reduction technique and data sample
The possible ways of measuring the age-metallicity relation for thegalactic disk in the neighborhood of the sun are discussed. It is shownthat the use of a field star sample chosen on the basis of effectivetemperature introduces a bias which results in a monotonic increase inthe metal abundance of the disk with time. However, if theage-metallicity relation for the disk can be shown to satisfy certaincriteria, the bias introduced in such a sample can be neglected: thegalactic disk apparently satisfies the criteria. It is concluded that asample analyzed through the use of uvby and H(beta) photometry inconjunction with a self-consistent set of theoretical isochronesprovides the least biased, most accurate estimate of the age-metallicityrelation for the disk.

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Dades d'Observació i Astrometria

Constel·lació:Carina
Ascensió Recta:09h17m26.92s
Declinació:-73°02'08.6"
Magnitud Aparent:8.114
Distancia:226.244 parsecs
Moviment propi RA:-15.8
Moviment propi Dec:21.4
B-T magnitude:8.367
V-T magnitude:8.135

Catàlegs i designacions:
Noms Propis
HD 1989HD 80866
TYCHO-2 2000TYC 9204-131-1
USNO-A2.0USNO-A2 0150-05913618
HIPHIP 45583

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