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Physical Processes of Interstellar Turbulence
Physical Processes Interstellar Turbulence self-gravity radiative heating
2012/2/23
I discuss the role of self-gravity and radiative heating and cooling in shaping the nature of the turbulence in the interstellar medium (ISM) of our galaxy. The heating and cooling cause it to be high...
Interstellar Turbulence and Star Formation
structure ISM clouds ISM magnetic fields turbulence methods numerical
2010/11/12
We provide a brief overview of recent advances and outstanding issues in simulations of interstellar turbulence, including isothermal models for interior structure of molecular clouds
and larger-scal...
Clouds and Instabilities in Supernova Remnant Structure：Interstellar Turbulence and Rippled Shocks
Supernova Remnant Structure Interstellar Turbulence Rippled Shocks
2009/6/16
Clouds and Instabilities in Supernova Remnant Structure：Interstellar Turbulence and Rippled Shocks。