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Analysis of MHD Simulations of the ISM (non-SCF)
We apply computer simulations of magnetohydrodynamics to analysis of the physics of the interstellar medium. We utilize mainly the simulations of Paolo Padoan and collaborators, which include radiative transfer and can generate realistic synthetic spectral-line maps of interstellar gas.

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Last modified on Monday, 22-Jan-2007 12:10:30 EST