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HD 208580


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The frequency analysis of low amplitude delta Scuti stars - VII. HD 208664.
Abstract image available at:http://adsabs.harvard.edu/abs/1982MNRAS.200..497K

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:Inder
Right ascension:21h59m16.58s
Declination:-62°28'36.8"
Apparent magnitude:8.152
Distance:184.502 parsecs
Proper motion RA:-0.8
Proper motion Dec:19.1
B-T magnitude:8.438
V-T magnitude:8.176

Catalogs and designations:
Proper Names   (Edit)
HD 1989HD 208580
TYCHO-2 2000TYC 9116-40-1
USNO-A2.0USNO-A2 0225-31360615
HIPHIP 108538

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