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Додај нови чланак| 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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| Сазвежђа: | Тукан |  | Ректацензија: | 23h17m54.48s |  | Deклинација: | -60°59'53.3" |  | Apparent магнитуда: | 8.135 |  | Даљина: | 130.378 parsecs |  | Proper motion RA: | -4.1 |  | Proper motion Dec: | 5.3 |  | B-T magnitude: | 8.536 |  | V-T magnitude: | 8.169 |  Каталог и designations:
 
 
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