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The chemical uniformity of stars in the same cluster is the result of turbulent mixing in the clouds of gas where star formation occurs, according to a study by astrophysicists at the University of Ca...
Recent high-angular-resolution (up to 0.7") dust polarization observations toward star forming regions are summarized. With the Sub-Millimeter Array, the emission from the dense structures is traced a...
The Galactic supernova remnant (SNR) IC443 is one of the most studied core-collapse SNRs for its interaction with molecular clouds. However, the ambient molecular clouds with which IC443 is interactin...
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 ...
The HII region IC 1848 harbors a lot of intricate elephant trunk-like structures that look morphologically different from usual bright-rimmed clouds (BRCs). Of particular interest is a concentration o...
We report the discovery and characterization of a power law correlation between the local surface densities of Spitzer-identified, dusty young stellar objects and the column density of gas (as traced ...
Supernova Remnants and Molecular Clouds     Supernova Remnants  Molecular Clouds       font style='font-size:12px;'> 2009/6/16
Supernova Remnants and Molecular Clouds
Clouds and Instabilities in Supernova Remnant Structure:Interstellar Turbulence and Rippled Shocks。
The Impact of Giant Stellar Outflows on their Clouds     Stellar Outflows  Clouds       font style='font-size:12px;'> 2009/6/15
The Impact of Giant Stellar Outflows on their Clouds

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