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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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Membre dels grups següents:
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Dades d'Observació i Astrometria
| Constel·lació: | Indus |
| Ascensió Recta: | 21h24m45.85s |
| Declinació: | -57°15'25.9" |
| Magnitud Aparent: | 7.188 |
| Distancia: | 254.453 parsecs |
| Moviment propi RA: | 37.2 |
| Moviment propi Dec: | -48.6 |
| B-T magnitude: | 7.445 |
| V-T magnitude: | 7.21 |
Catàlegs i designacions:
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