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Clustered Star Formation in Magnetic Clouds: Properties of Dense Cores Formed in Outflow-Driven Turbulence
Magnetic Clouds: Properties Dense Cores Formed Outflow-Driven Turbulence
2011/10/11
We investigate the physical properties of dense cores formed in turbulent, magnetized, parsec-scale clumps of molecular clouds, using three-dimensional numerical simulations that include protostellar ...
Dense Molecular Gas Clumps Associated with Clustered Star Formation in the Rosette Molecular Cloud
Dense Molecular Gas Clumps Rosette Molecular Cloud Clustered Star Formation
2009/6/16
Dense Molecular Gas Clumps Associated with Clustered Star Formation in the Rosette Molecular Cloud。