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Observations of Molecules in High Redshift Galaxies

Published online by Cambridge University Press:  21 December 2011

Kirsten Kraiberg Knudsen
Kirsten Kraiberg Knudsen*
Affiliation:
Department of Earth and Space Sciences, Chalmers University of Technology, Onsala Space Observatory, SE-439 92 Onsala, Sweden email: kraiberg@chalmers.se
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Abstract

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I present an overview of the molecular gas observations in high redshift galaxies. This field has seen tremendous progress in the past few years, with an increased number of detections of other molecules than CO. The molecular line observations are done towards different classes of massive starbursts, including submillimeter galaxies, quasars, and massive gas-rich disks. I will highlight results of detections of HCN, HCO+, and other small molecules, as well as the Spitzer detections of PAHs. Additionally, I will discuss about the excitation of CO and other species in the high-z galaxies and put this in the context of new telescopes such as ALMA.

Keywords

ISM: moleculesgalaxies: evolutiongalaxies: ISMgalaxies: high-redshiftgalaxies: starburstquasars: emission linesinfrared: ISMradio lines: galaxiessubmillimeter
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 7 , Symposium S280: The Molecular Universe , June 2011 , pp. 325 - 338
Copyright
Copyright © International Astronomical Union 2011

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