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Dense core formation by fragmentation of velocity-coherent filaments in L1517
Stars: formation - ISM: clouds - molecules - kinematics and dynamics - structure - Radio lines: ISM
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2011/9/28
Context. Low-mass star-forming cores differ from their surrounding molecular cloud in turbulence, shape, and density structure. Aims. We aim to understand how dense cores form out of the less dense cl...
Star Formation from Gravoturbulent Fragmentation
Star Formation Gravoturbulent Fragmentation
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2009/6/16
Star Formation from Gravoturbulent Fragmentation。