Astronomy and Astrophysics – Astrophysics
Scientific paper
2001-04-17
Astronomy and Astrophysics
Astrophysics
AASTeX, 19 pages, 15 figures; final, revised version; accepted to ApJ
Scientific paper
10.1086/323952
We have computed line emission cooling rates for the main cooling species in models of interstellar molecular clouds. The models are based on numerical simulations of super-sonic magneto-hydrodynamic (MHD) turbulence. Non-LTE radiative transfer calculations have been performed to properly account for the complex density and velocity structures in the MHD simulations. Three models are used. Two of the models are based on MHD simulations with different magnetic field strength and the third includes the computation of self-gravity (in the super-Alfvenic regime of turbulence). The density and velocity fields in the simulations are determined self-consistently by the dynamics of super-sonic turbulence. The models are intended to represent molecular clouds with linear size L~6 pc and mean density
Juvela Mika
Nordlund Aake
Padoan Paolo
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