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REVEALING A DETAILED MASS DISTRIBUTION OF A HIGH-DENSITY CORE MC27/L1521F IN TAURUS WITH ALMA

  • Authors: Kazuki Tokuda, Toshikazu Onishi, Tomoaki Matsumoto, Kazuya Saigo, Akiko Kawamura, Yasuo Fukui, Shu-ichiro Inutsuka, Masahiro N. Machida, Kengo Tomida, Kengo Tachihara, and Philippe André

2016 The Astrophysical Journal 826 26.

  • Provider: AAS Journals

Caption: Figure 2.

Distribution of 1.2 mm dust continuum emission toward MC27/L1521F. (a) Both color scale and contours show 1.2 mm dust continuum images obtained by the 7 m array. The lowest contour and subsequent contour step are 3.6 mJy beam−1. (b) Both color scale and contours show 1.2 mm dust continuum images obtained by the 12 m array. The lowest contour and subsequent contour step are 0.3 mJy beam−1. The angular resolutions are given by ellipses in the lower left corner of each panel. Black crosses in each panel represent the position of the Spitzer source.

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