Methanol: a diagnostic tool for high-mass star-forming regions

Details Methanol: a diagnostic tool for high-mass star-forming regions Methanol: a diagnostic tool for high-mass star-forming regions

2004-02-01

arxiv.org/abs/astro-ph/0402014v1

Astron.Astrophys. 422 (2004) 573-585

Astronomy and Astrophysics

Astrophysics

4 pages, 2 figures. (Co)authored by members of the MPIfR (Sub)millimeter Astronomy Group. To appear in the Proceedings of the

Scientific paper

We here present an innovative technique to handle the problem of deriving
physical parameters from observed multi-line spectra of methanol, based on the
simultaneous fit of all the lines with a synthetic spectrum computed under the
Large Velocity Gradient approximation; the best physical parameters are found
using numerical methods.

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