High Redshift CO Line Emission:. Perspectives

Details High Redshift CO Line Emission:. Perspectives High Redshift CO Line Emission:. Perspectives

Oct 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001dms..conf..109c&link_type=abstract

DEEP MILLIMETER SURVEYS Implications for Galaxy Formation and Evolution. Held 19-21 June 2000 in University of Massachusetts, Am

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Although about a dozen high redshift (z > 2) starburst galaxies have been recently detected in the CO lines, spectroscopic detections of molecular gas of very young galaxies are still very difficult. The CO lines are usually optically thick, which limits greatly the increase of emission with redshift, as observed for the dust continuum. This paper discusses the significant progress that future instruments (LMT, ALMA) will make in this area. The computations are based on an extrapolation of our understanding of starburst galaxies at lower redshift.

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