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The CO-to-H2 Conversion Factor from Infrared Dust Emission across the Local Group

  • Authors: Adam K. Leroy, Alberto Bolatto, Karl Gordon, Karin Sandstrom, Pierre Gratier, Erik Rosolowsky, Charles W. Engelbracht, Norikazu Mizuno, Edvige Corbelli, Yasuo Fukui, and Akiko Kawamura

Leroy et al. 2011 The Astrophysical Journal 737 12.

  • Provider: AAS Journals

Caption: Figure 3.

Scatter plots showing Σ gas as a function of Σ dust for M 31. The columns show the relationship between dust ( x-axis) and (left) H i, (middle) H 2 derived from CO using our best-fit α CO, and (right) total (H i + H 2) gas. Our best-fit α CO yields reasonable linear scalings between total gas and dust in each system (the red line shows the median δ GDR), usually a clear improvement on the relationship between dust and either phase alone.

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