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Properties of Bulgeless Disk Galaxies. II. Star Formation as a Function of Circular Velocity

  • Authors: Linda C. Watson, Paul Martini, Ute Lisenfeld, Man-Hong Wong, Torsten Böker, and Eva Schinnerer

Watson et al. 2012 The Astrophysical Journal 751 123.

  • Provider: AAS Journals

Caption: Figure 4.

SFR surface density vs. molecular hydrogen surface density. Symbols are as in Figure 3. The solid line shows the Bigiel et al. (2008) fit to the molecular hydrogen star formation law: . We discuss the offset of our data relative to this fit in Section 4.1.2.

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