Figure 19 from Extending the Nearby Galaxy Heritage with WISE: First Results from the WISE Enhanced Resolution Galaxy Atlas

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Extending the Nearby Galaxy Heritage with WISE: First Results from the WISE Enhanced Resolution Galaxy Atlas

Authors: T. H. Jarrett, F. Masci, C. W. Tsai, S. Petty, M. E. Cluver, Roberto J. Assef, D. Benford, A. Blain, C. Bridge, E. Donoso, P. Eisenhardt, B. Koribalski, S. Lake, James D. Neill, M. Seibert, K. Sheth, A. Stanford, and N. Wright

Jarrett et al. 2013 The Astronomical Journal 145 6.

Provider: AAS Journals

Caption: Figure 19.

sSFR compared to the Hubble type and stellar mass. The stellar mass is derived using the M/ L relation from this work (Equation (9)). Two global SFRs are shown: black points correspond to the SFR (22 μm; Equation (2)) and blue squares correspond to the combined IR+UV SFR. There is a similar linear trend (illustrated by the blue shaded regions) for both Hubble type and the host stellar mass. A range in SFRs (from 0.1 to 10 M _☉ yr ⁻¹) are represented by the dashed lines.

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