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Low CO Luminosities in Dwarf Galaxies

  • Authors: Andreas Schruba, Adam K. Leroy, Fabian Walter, Frank Bigiel, Elias Brinks, W. J. G. de Blok, Carsten Kramer, Erik Rosolowsky, Karin Sandstrom, Karl Schuster, Antonio Usero, Axel Weiss, and Helmut Wiesemeyer

Schruba et al. 2012 The Astronomical Journal 143 138.

  • Provider: AAS Journals

Caption: Figure 6.

Metallicity dependence of the CO-to-H 2 conversion factor. α CO is derived from the ratio of observed SFR scaled by a constant H 2 depletion time, τ dep = 1.8 Gyr, and the observed CO luminosity, L CO. Bigger symbols show galaxy-integrated measurements of dwarf galaxies from this work; smaller symbols show data for our literature compilation with starbursts highlighted by stars. The horizontal dashed line shows the Galactic conversion factor, and the diagonal lines show regression fits: to all galaxies (dotted line), to all non-starburst galaxies (dashed line), and exclusively to the HERACLES sample (solid line).

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