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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 5.

SFR surface density vs. total hydrogen surface density. Symbols are as in Figure 3. The magenta dot-dashed line shows the Kennicutt (1998) fit to a sample of 61 normal spirals and 36 starburst galaxies, where the measurements are averages over the optical disk. The dotted line shows the Kennicutt et al. (2007) fit to M51 data at 520 pc resolution. The solid black line shows the Krumholz et al. (2009) model at 0.4  Z metallicity.

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