Fig. 5 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

Authors: Yancy L. Shirley, Neal J. Evans II, and Jonathan M. C. Rawlings

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

Provider: AAS Journals

Caption: Fig. 5.

Best‐fit power‐law model for B335. The parameters of the best fit were ﹩p=1.8﹩, ﹩n_{f}=1.5\times 10^{6}﹩ cm⁻³, ﹩L_{\mathrm{int}\,}=3.3﹩ L_⊙, and ﹩s_{\mathrm{ISRF}\,}=0.3﹩.

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