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HD 20094


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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:Ωρολόγιον
Right ascension:03h10m22.63s
Declination:-63°15'14.0"
Apparent magnitude:8.217
Distance:181.818 parsecs
Proper motion RA:2.7
Proper motion Dec:-11.7
B-T magnitude:8.599
V-T magnitude:8.249

Catalogs and designations:
Proper Names   (Edit)
HD 1989HD 20094
TYCHO-2 2000TYC 8863-1061-1
USNO-A2.0USNO-A2 0225-00795731
HIPHIP 14744

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