Latitude Variation and Greenwich Observations, 1851-91
نویسندگان
چکیده
منابع مشابه
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Our galaxy is a spiral galaxy and its stars are mostly in a thin disk and rotate around the galactic center. The vertical component of the dispersion velocity of stars is a function of the galactic latitude and decreases with increasing it. In the galactic Besancon model, this dependence is ignored and they just consider the dependence of dispersion velocity on the stellar age. Becanson model i...
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ژورنال
عنوان ژورنال: Monthly Notices of the Royal Astronomical Society
سال: 1893
ISSN: 0035-8711,1365-2966
DOI: 10.1093/mnras/53.3.120