CO Emission from High Redshift Galaxies

Details CO Emission from High Redshift Galaxies CO Emission from High Redshift Galaxies

Aug 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999pcim.conf...10s&link_type=abstract

The Physics and Chemistry of the Interstellar Medium, Proceedings of the 3rd Cologne-Zermatt Symposium, held in Zermatt, Septemb

Physics

Scientific paper

Theoretical results are presented for the CO emissivity of star forming
galaxies at high redshift. It is found that actively star forming
galaxies should be detectable, if they indeed exist, with the MMA out to
redshifts of 20. The interplay between the ambient warm CMB and the
thermal balance of PDRs is emphasized.

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