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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...
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。