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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 1.

Coverage of CO observations. For each HERACLES dwarf galaxy we show the coverage of our CO data (gray dashed line), the H i surface density (gray scale) at linear scale between 0 and 40  M  pc −2, the 24 μm intensity (red contour) at 0.2 MJy sr −1, the FUV intensity (blue contour) at 0.01 MJy sr −1, and a galactocentric radius R = R 25 (white contour). We determine the CO intensity at each sampling point (dot) and stack the data for the "entire" galaxy (black contour) and for IR-bright regions (red contour); see the text for definition of stacking regions.

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