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HD 24136


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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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观测天体数据

星座:網罟座
右阿森松:03h46m15.62s
赤纬:-66°30'14.7"
视星:7.686
距离:202.429 天文距离
右阿森松适当运动:-14.2
赤纬适当运动:-23.9
B-T magnitude:8.119
V-T magnitude:7.722

目录:
适当名称   (Edit)
HD 1989HD 24136
TYCHO-2 2000TYC 8873-998-1
USNO-A2.0USNO-A2 0225-00945548
HIPHIP 17604

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