Fig. 1 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. 1.

Beam profiles used for modeling Class 0 sources. The beam profile from 1998 January to 1998 April and Gaussian beams with the FWHMs reported in Paper I are shown. Since CRL 618 is a weak calibrator, the 1998 January beam was extrapolated beyond 34^{﹩\arcsec﹩} using the 1998 April beam.

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