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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 3.

SFR surface density vs. atomic hydrogen surface density. Red squares represent galaxies with v circ < 120 km s −1. Blue triangles represent galaxies with v circ > 120 km s −1. The circular velocities are from H i rotation curve fits (Paper I). A representative error bar is shown in the lower right corner (see Sections 3.1 and 3.2 for details). The vertical dashed line is at 9  M  pc −2, the typical maximum density for atomic hydrogen. For comparison, the small black points represent measurements from Bigiel et al. (2008) from seven spiral galaxies sampled at 750 pc resolution.

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