Characterizing the Extreme Star-Formation Environment in Arp 220

Details Characterizing the Extreme Star-Formation Environment in Arp 220 Characterizing the Extreme Star-Formation Environment in Arp 220

Nov 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011eas....52..297r&link_type=abstract

EAS Publications Series, Volume 52, 2011, pp.297-298

Physics

Scientific paper

We present a full spectral view of Arp 220 from 450 GHz to 1500 GHz
using Herschel SPIRE. The non-LTE modeling of mid-J to high-J CO lines
suggests surprisingly warm molecular gas between 500 and 1500 K, the
mass of which is about 1% of the cold gas mass.

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