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Gas Kinematics of the Massive Protocluster G286.21+0.17 Revealed by ALMA

  • Authors: Yu Cheng, Jonathan C. Tan, Mengyao Liu, Wanggi Lim, and Morten Andersen

2020 The Astrophysical Journal 894 87.

  • Provider: AAS Journals

Caption: Figure 6.

The 7 m C18O(2–1) emission integrated over 0.5 km s−1 intervals, as indicated in the upper left corner of each panel, from −22.0 to −17.0 km s−1. The black contours show the 7 m array 1.3 mm continuum emission. The contour levels are 1.7 mJy beam−1 × (4, 10, 20, 50, 100).

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