Model results for shocked gas in active star forming regions

Details Model results for shocked gas in active star forming regions Model results for shocked gas in active star forming regions

Dec 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007msl..confe.100k&link_type=abstract

"Molecules in Space and Laboratory, meeting held in Paris, France, May 14-18, 2007. Editors: J.L. Lemaire, F. Combes. ISBN: 9782

Astronomy and Astrophysics

Astrophysics

Modelling_Environments

Scientific paper

In order to compare recent observations of shocks in the interstellar medium with models, we have run a large grid of 25 000 shock models. These models are very sophisticated and includes a very detailed chemistry. We use the results from this grid to reproduce observations of a bow shock located in the Orion Molecular Cloud. In doing that we are constraining physical conditions in an active star forming region.

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