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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 12.

Left: SFR surface density vs. total hydrogen surface density, as in Figure 5, but showing a larger range to demonstrate the model trends. The data are divided by oxygen abundance, where orange pentagons represent galaxies with 12 + log (O/H) < 8.7 and purple circles represent galaxies with 12 + log (O/H) > 8.7. The lines show the Krumholz et al. (2009) model with a metallicity of 0.1  Z (orange solid) and 1.4  Z (purple dashed), which corresponds to the lowest and highest metallicities in our sample. Right: histograms of the offset of the data from the Krumholz et al. (2009) model with a metallicity of 0.4  Z . The orange line represents the distribution of galaxies with 12 + log (O/H) < 8.7 and the purple line represents the distribution of galaxies with 12 + log (O/H) > 8.7. There is no significant difference between the distributions.

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