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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 11.

Trend of q 24 = log[ f ν(24 μm)/ f ν(1.4 GHz)] with log( L(TIR)). The line shows our preferred fit, a constant of q 24=1.22 for log( L(TIR)) < 11, and a sloping line above.

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