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HD 169979


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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:Ταώς
Right ascension:18h33m47.45s
Declination:-71°46'07.0"
Apparent magnitude:7.002
Distance:90.992 parsecs
Proper motion RA:-3.6
Proper motion Dec:8.1
B-T magnitude:7.323
V-T magnitude:7.029

Catalogs and designations:
Proper Names   (Edit)
HD 1989HD 169979
TYCHO-2 2000TYC 9299-2362-1
USNO-A2.0USNO-A2 0150-18512891
HIPHIP 90997

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