CO Line SEDs in Local Luminous Infrared Galaxies

Details CO Line SEDs in Local Luminous Infrared Galaxies CO Line SEDs in Local Luminous Infrared Galaxies

Oct 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aspc..408...86a&link_type=abstract

The Starburst-AGN Connection. ASP Conference Series, Vol. 408, proceedings of the conference held 27-31 October 2008, at Shangha

Astronomy and Astrophysics

Astronomy

Scientific paper

A small sample of 5 bright luminous infrared galaxies (LIRGs) was observed and the ço\ mapping results reveal the gas distribution concentrated on the galactic nuclei. For NGC 3256, the maps in the CO(3-2), (4-3) and (6-5) transitions were obtained. Together with the measurements in the lower transitions from the literatures, the peak of the CO line spectral energy distribution was found at CO(5-4). Local LIRG NGC 3256 shows slightly lower excitation conditions than the submm galaxies (SMGs).

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