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CHAOS. III. GAS-PHASE ABUNDANCES IN NGC 5457

  • Authors: Kevin V. Croxall, Richard W. Pogge, Danielle A. Berg, Evan D. Skillman, and John Moustakas

2016 The Astrophysical Journal 830 4.

  • Provider: AAS Journals

Caption: Figure 4.

Plots of T[O II] against T[N II] (top) and T[S II] against T[N II] (bottom) measured for H II regions in NGC 5457. The dashed one-to-one line plotted shows that the data are in agreement with these ions being isothermal.

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