Figure 8 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 8.

Trend of L(24)/ L _tot(IR) with L(TIR). L(TIR) is based strictly on the formulation of Sanders et al. (2003) using IRAS data, while L _tot(IR) is obtained by integrating under the infrared SED from 5 to 1000 μm.

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