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Theory of formation of massive stars via accretionA semi-analytical scheme for augmenting existing evolutionary tracks of pre-main sequence protostars is introduced and discussed.
Document ID
20060032064
Acquisition Source
Jet Propulsion Laboratory
Document Type
Conference Paper
External Source(s)
hdl:2014/13494
Authors
Yorke, H. W.
Date Acquired
August 23, 2013
Publication Date
August 6, 2001
Subject Category
Astronomy
Distribution Limits
Public
Copyright
Other
Keywords
star formation

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