Finding binary star fractions in any distribution
نویسندگان
چکیده
منابع مشابه
On the origin of the distribution of binary - star periods
Pre-main sequence and main-sequence binary systems are observed to have periods, P , ranging from one day to 10 days and eccentricities, e, ranging from 0 to 1. We pose the problem if stellar-dynamical interactions in very young and compact star clusters may broaden an initially narrow period distribution to the observed width. N -body computations of extremely compact clusters containing 100 a...
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ژورنال
عنوان ژورنال: Monthly Notices of the Royal Astronomical Society
سال: 2019
ISSN: 0035-8711,1365-2966
DOI: 10.1093/mnras/stz1939