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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 8.

Fits to simulated data. The y-axis gives the mean best-fit α CO divided by the true value (known by construction) as a function of the intrinsic scatter in the dust–gas relation ( x-axis). Error bars show the rms scatter in the best-fit α CO. The horizontal line at 1 shows a perfect match between true and best-fit α CO. Different colors indicate different systems. For realistic intrinsic scatter (≲ 0.2 dex, see Table 2), we recover the true α CO with better than 40% accuracy in all cases.

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