The Short-Period Binary Frequency Among Low-Mass Pre-Main Sequence Stars
نویسندگان
چکیده
منابع مشابه
The Rotation of Low-Mass Pre-Main-Sequence Stars
Major photometric monitoring campaigns of star-forming regions in the past decade have provided rich rotation period distributions of pre-main-sequence stars. The rotation periods span more than an order of magnitude in period, with most falling between 1 and 10 days. Thus the broad rotation period distributions found in 100 Myr clusters are already established by an age of 1 Myr. The most rapi...
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ژورنال
عنوان ژورنال: International Astronomical Union Colloquium
سال: 1992
ISSN: 0252-9211
DOI: 10.1017/s0252921100006084