Figure 10 from Properties of Bulgeless Disk Galaxies. II. Star Formation as a Function of Circular Velocity

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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 10.

Stability parameter, including the gas and stellar contribution, vs. circular velocity. There is no circular velocity at which a transition in stability occurs. We describe our derivation of the vertical error bar in Section 3.4.

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