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HD 37940


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Flamsteed stars not contained in the Yale "Catalogue of Bright Stars"
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Physical parameters of pulsating variables with periods between one and three days. I - Photometry and metallicities
Based on a new set of observations in the Walraven VBLUW system,obtained at the European Southern Observatory, La Silla, Chile,Fe/H(VBLU) values of 57 pulsating variables, mostly with periods betweenone and three days,. are determined. The distribution of the metalabundances is shown to be essentially bimodal. All the variables withFe/H ratios of less than -0.4 were classified by Diethelm (1983) as RRdstars. They are identified as the galactic field counterpart of theCepheids in the same period range found in globular clusters.

Determination of omega and IOTA values for rotating BO-B3 stars. I.
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Observations of occultations made at the University observatory at Brno in the years 1961-1962
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观测天体数据

星座:金牛座
右阿森松:05h42m53.67s
赤纬:+18°58'49.3"
视星:6.648
距离:119.048 天文距离
右阿森松适当运动:-6
赤纬适当运动:-11.9
B-T magnitude:6.641
V-T magnitude:6.648

目录:
适当名称   (Edit)
HD 1989HD 37940
TYCHO-2 2000TYC 1306-932-1
USNO-A2.0USNO-A2 1050-02443588
HIPHIP 26925

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