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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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Observation and Astrometry data
| Constellation: | Indien |
| Right ascension: | 21h20m38.74s |
| Declination: | -57°50'55.5" |
| Apparent magnitude: | 7.807 |
| Distance: | 153.139 parsecs |
| Proper motion RA: | 7.4 |
| Proper motion Dec: | 8.7 |
| B-T magnitude: | 8.128 |
| V-T magnitude: | 7.834 |
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