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We analyze the HCO+ 3-2 and H13CO+ 3-2 line profiles of 27 high-mass star-forming regions to identify asymmetries that are suggestive of mass inflow. Three quantitative measures of line asymmetry are ...
The annihilation of the dark matter in clumps around cosmic string loops is studied. These clumps form at the radiation dominated stage and may have densities \gg\rho_{eq}. We conclude that 100 GeV ne...
We study the mass-density relationship n m^x in molecular cloud clumps, considering various relations between the gravitational, kinetic, internal and magnetic energy. Clumps are described statistical...
Many observed massive star-forming z ≈ 2 galaxies are large disks that exhibit irregular morphologies, with ≈ 1 kpc, ≈ 108-10M⊙ clumps. We present high-resolution cosmological SPH simulations that zoo...
Shadows and photoevaporated flows from neutral clumps exposed to two ionizing sources。
3D Simulations of the Fragmentation of Photoevaporating Clumps Embedded in a Stellar Wind。
Numerical simulations of the fragmentation of photoevaporating nonuniform clumps
Dense Molecular Gas Clumps Associated with Clustered Star Formation in the Rosette Molecular Cloud。
HH Illumination of Clumps within Molecular Clouds。

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