Molecular line diagnostics of feeding and feedback in starburst and AGN galaxies

Details Molecular line diagnostics of feeding and feedback in starburst and AGN galaxies Molecular line diagnostics of feeding and feedback in starburst and AGN galaxies

Dec 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007msl..confe..40u&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

Observations

Scientific paper

Radiation fields and kinematical perturbations can modify the chemical composition of the molecular interstellar medium in starburst and AGN galaxies. We have characterized the molecular chemistry in two star-forming (IC 342, M 82) and one AGN (NGC 1068) nearby galaxies through multispecies observations. The gas composition in these sources is driven by shocks, UV radiation or X-rays across hundreds of parsecs. Molecular line observations have the potential to unveil gas processing by the feeding and feedback mechanisms that drive the evolution of starburst and AGN episodes.

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