Figure 15 from Determining Star Formation Rates for Infrared Galaxies

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Determining Star Formation Rates for Infrared Galaxies

Authors: G. H. Rieke, A. Alonso-Herrero, B. J. Weiner, P. G. Pérez-González, M. Blaylock, J. L. Donley, and D. Marcillac

RIEKE et al. 2009 The Astrophysical Journal 692 556.

Provider: AAS Journals

Caption: Figure 15.

Comparison of L(24) and L(TIR). The line is a linear fit as given in the text. It fits well with virtually no outliers and with a slope close to one ( L(TIR) = 27.9 L(24) ^0.945). Symbols are as for Figure 13.

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