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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 9.

SFE ( ) vs. stability parameters Q gas (left), Q stars (middle), and Q gas + stars, min (right). The symbols are as in Figure 3. Note that the condition for instability is Q ≲ 1, so none of our galaxies are strictly unstable. We describe our derivation of the error bar in Sections 3.2 and 3.4.

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