Applying the Meudon PDR code on dense structures from MHD simulations of the ISM

Details Applying the Meudon PDR code on dense structures from MHD simulations of the ISM Applying the Meudon PDR code on dense structures from MHD simulations of the ISM

May 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011iaus..280p.233l&link_type=abstract

The Molecular Universe, Posters from the proceedings of the 280th Symposium of the International Astronomical Union held in Tole

Astronomy and Astrophysics

Astronomy

Scientific paper

We present results of the application of the one-dimensional Meudon PDR code to selected lines of sight within an MHD simulation of the ISM. The simulation describes the head-on collision of two flows of WNM, leading to the formation of cold and dense structures within a much warmer and more tenuous medium, via atomic cooling and self-gravity. The application of the PDR code to density profiles extracted from this simulation allows us to describe the chemical structure of dense cores, in particular putting forward further theoretical evidence for a "dark" (i.e. not seen in CO) component of the molecular gas.

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