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HD 4510


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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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Osservazione e dati astrometrici

Costellazione:Tucano
Ascensione retta:00h46m16.80s
Declinazione:-62°40'32.8"
Magnitudine apparente:7.713
Distanza:171.821 parsec
Moto proprio RA:63.3
Moto proprio Dec:-17.9
B-T magnitude:8.025
V-T magnitude:7.739

Cataloghi e designazioni:
Nomi esatti   (Edit)
HD 1989HD 4510
TYCHO-2 2000TYC 8845-890-1
USNO-A2.0USNO-A2 0225-00202248
HIPHIP 3614

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