Modelling the chemistry of external galaxies

Details Modelling the chemistry of external galaxies Modelling the chemistry of external galaxies

Dec 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007msl..confe..97b&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

Astrochemistry for the Milky Way is fairly well understood, but external galaxies where the physical conditions are different from those in the Milky Way may have different molecular tracers. We present results from two studies; first, calculations of the CO to H2 conversion factor for different galaxies and, second, calculations of hot core tracer abundances for the physical conditions expected in external galaxies.

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