Fig. 13 from Tracing the Mass during Low‐Mass Star Formation. III. Models of the Submillimeter Dust Continuum Emission from Class 0 Protostars

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

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. 13.

Ratio of specific intensity, ﹩I^{\mathrm{norm}\,}_{450}/ I^{\mathrm{norm}\,}_{850}﹩ for the best‐fit power‐law models of isolated Class 0 sources (solid line). Points are spaced at the half‐beam resolution at 850 μm.

Other Images in This Article

Copyright and Terms & Conditions