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Implications of Binary Properties for Theories of Star Formation

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arxiv astro-ph/0006288 v1 pith:JWIKIUZU submitted 2000-06-20 astro-ph

Implications of Binary Properties for Theories of Star Formation

classification astro-ph
keywords formationstarstarsaccretionbinarycloseinteractionsother
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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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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