Astronomy and Astrophysics – Astrophysics
Scientific paper
2000-06-20
Published in "The Formation of Binary Stars", IAU Symposium 200, eds. H. Zinnecker and R. D. Mathieu (ASP, San Francisco, 2001
Astronomy and Astrophysics
Astrophysics
12 pages, text only, presented at IAU Symposium 200, "The Formation of Binary Stars", Potsdam, Germany, April 10-15, 2000; to
Scientific paper
The overall frequency and other statistical properties of binary systems suggest that star formation is intrinsically a complex and chaotic process, and that most binaries and single stars actually originate from the decay of multiple systems. Interactions between stars forming in close proximity to each other may play an important role in the star formation process itself, for example via tidally induced accretion from disks. Some of the energetic activity of newly formed stars could be due to bursts of rapid accretion triggered by interactions with close companions.
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