Turbulence in the Interstellar Medium |
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Authors: | Mordecai-Mark MacLow |
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Affiliation: | 1. Department of Astrophysics, American Museum of Natural History, New York, NY, 10024-5192, USA
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Abstract: | Interstellar turbulence is expected to dissipate quickly in theabsence of continuous energy input. I examine the energy availablefor driving the turbulence from six likely mechanisms:magnetorotational instability, gravitational instability, protostellaroutflows, HII region expansion, stellar winds, and supernovae.I conclude that supernovae contribute far more energy than the othermechanisms, and so form the most likely drving mechanism. |
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