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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
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...
The Jeans Mass as a Fundamental Measure of Self-Gravitating Disc Fragmentation and Initial Fragment Mass
stars: formation accretion accretion discs methods:analytical
2011/9/28
As a formation route for objects such as giant planets and low-mass stars in protostellar discs (as well as stars in AGN discs), theories of self-gravitating disc fragmentation need to be able to pred...
Star Formation from Gravoturbulent Fragmentation
Star Formation Gravoturbulent Fragmentation
2009/6/16
Star Formation from Gravoturbulent Fragmentation。
Recent Advances in the Collapse and Fragmentation of Turbulent Molecular Cloud Cores
Collapse Turbulent Molecular Cloud Cores Fragmentation
2009/6/15
Recent Advances in the Collapse and Fragmentation of Turbulent Molecular Cloud Cores。