Fig. 4 from Tracing the Mass during Low‐Mass Star Formation. III. Models of the Submillimeter Dust Continuum Emission from Class 0 Protostars

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Tracing the Mass during Low‐Mass Star Formation. III. Models of the Submillimeter Dust Continuum Emission from Class 0 Protostars

Shirley, Evans, & Rawlings 2002 The Astrophysical Journal 575 337.

Caption: Fig. 4.

Effects of changing the strength of the ISRF. Three ﹩p=2﹩ power‐law models of B335 are shown with ﹩s_{\mathrm{ISRF}\,}=0.3﹩, 1.0, and 3.0.