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The CO-H2 Conversion Factor in Galaxy Mergers

By Desika Narayanan

Abstract

The CO-H2 conversion factor in galaxies is typically described as bimodal: one value for discs and quiescent regions, and another (lower) value for mergers and starbursts. In this proceeding, I will describe both empirical observational evidence that the conversion factor varies with physical environment, as well as a theoretical model which aims to understand the physical processes which drive these variations. I present a functional form for Xco which can be applied to observations ranging in scale from ~70 pc to galaxy-wide scales, and show the consequences of the application of this model to the Kennicutt-Schmidt star formation law.Comment: Conference Proceedings for Galaxy Mergers in an Evolving Universe (Hualien, Taiwan); Editors: Wei-Hsin Sun, Nick Scovill

Topics: Astrophysics - Cosmology and Nongalactic Astrophysics
Year: 2011
OAI identifier: oai:arXiv.org:1112.1073

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