Figure 1 from INTERFEROMETRIC MAPPING OF MAGNETIC FIELDS: THE ALMA VIEW OF THE MASSIVE STAR-FORMING CLUMP W43-MM1

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INTERFEROMETRIC MAPPING OF MAGNETIC FIELDS: THE ALMA VIEW OF THE MASSIVE STAR-FORMING CLUMP W43-MM1

Authors: Paulo C. Cortes, Josep M. Girart, Charles L. H. Hull, Tirupati K. Sridharan, Fabien Louvet, Richard Plambeck, Zhi-Yun Li, Richard M. Crutcher, and Shih-Ping Lai

2016 The Astrophysical Journal Letters 825 L15.

Provider: AAS Journals

Caption: Figure 1.

Stokes I emission from the W43_MM1 clump indicated by the colorscale in Jy ﹩{\mathrm{beam}}^{-1}﹩. Overlaid are the sources extracted as ellipses, in black, representing the deconvolved sized obtained from the Gaussian fits. With an rms noise of ﹩\sigma =0.41﹩ mJy ﹩{\mathrm{beam}}^{-1}﹩, the dynamic range of the self-calibrated image is 1220.

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