Non-LTE line formation in clumpy and turbulent molecular clouds
M. Hegmann and
Received 2 February 2000 / Accepted 4 May 2000
Extending previous work (Albrecht & Kegel 1987, Kegel et al. 1993, Piehler & Kegel 1994), we investigated the formation of interstellar molecular lines in a medium with stochastic density and velocity fluctuations. We solved the full NLTE-problem, i.e. the generalized radiative transfer equation simultaneously with the rate equations, for a 6-level CO molecule and a plane-parallel slab geometry. Our results indicate that accounting for a finite correlation length of both, the density and velocity field, strongly affects the line profile and the line width as well as the intensity ratios of different rotational transitions.
Key words: line: formation radiative transfer ISM: clouds ISM: molecules radio lines: ISM
Send offprint requests to: M. Hegmann (Hegmann@astro.uni-frankfurt.de)
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© European Southern Observatory (ESO) 2000
Online publication: June 30, 2000