THE LOW-MASS ASTROMETRIC BINARY LSR 1610–0040
نویسندگان
چکیده
منابع مشابه
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In a previous paper (Martin et al., 1997) we have shown that for double stars with orbital periods smaller than about 25 years, it was possible to determine from the Hipparcos data, the mass ratio B of the components or the difference between the mass and intensity ratios, β−B, provided the orbital elements of the relative orbit are available. Froman extensive literature search we have selected...
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ژورنال
عنوان ژورنال: The Astronomical Journal
سال: 2016
ISSN: 1538-3881
DOI: 10.3847/0004-6256/151/3/57