Figure 2 from LIGHTING THE DARK MOLECULAR GAS: H2 AS A DIRECT TRACER

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LIGHTING THE DARK MOLECULAR GAS: H₂ AS A DIRECT TRACER

Authors: Aditya Togi, and J. D. T. Smith

2016 The Astrophysical Journal 830 18.

Provider: AAS Journals

Caption: Figure 2.

Frequency distribution of the power-law index, n, required to fit the MIR ﹩{{\rm{H}}}_{2}﹩ rotational lines. The average value ﹩\bar{n}=4.84\pm 0.61﹩ for the SINGS galaxy sample.

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