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HD 127296


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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.

Photometry of bright southern cepheids
Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1970MNRAS.148....1S&db_key=AST

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观测天体数据

星座:豺狼座
右阿森松:14h32m30.98s
赤纬:-55°27'49.6"
视星:7.378
距离:126.904 天文距离
右阿森松适当运动:-24.1
赤纬适当运动:-3.5
B-T magnitude:7.714
V-T magnitude:7.406

目录:
适当名称   (Edit)
HD 1989HD 127296
TYCHO-2 2000TYC 8683-1178-1
USNO-A2.0USNO-A2 0300-21513498
HIPHIP 71112

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