Molecular Emission in LIRGs and ULIRGs

Details Molecular Emission in LIRGs and ULIRGs Molecular Emission in LIRGs and ULIRGs

Oct 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004mas..conf..103v&link_type=abstract

MULTIWAVELENGTH AGN SURVEYS. Proceedings of the Guillermo Haro Conference 2003. Held 8-12 December 2003 in Cozumel, Mexico. Edit

Astronomy and Astrophysics

Astronomy

Scientific paper

We study the properties of dust and molecular gas in a sample of 6 Luminous Infrared Galaxies (LIRGs and ULIRGs). For the analysis we use a new method that combines the dust emission models provided by GRASIL with one-zone molecular emission models. The analysed galaxies show a tight correlation between the molecular gas temperature and the Radio and FIR luminosity. NGC7469, a Sy1 galaxy, stands clearly out of the relation, suggesting a new way to detect dust enshrouded AGN.

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