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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 3.

(a) Channel maps of TP CO(2–1) emission integrated over every 2.0 km s−1, as indicated in the upper left corner of each panel (indicating the central velocity of the range), from −55.0 to +15.0 km s−1. The contour levels are 1 Jy beam−1 km s−1 × (1, 5, 10, 20, 40, 80, 200). The red plus sign in each panel marks the phase center of the observation (R.A. = 10:38:33, decl. = −58:19:22). The thick black contour in the lower left panel shows the 4σ level of the 7 m continuum emission. (b) Channel maps of TP C18O(2–1) emission integrated over every 1.0 km s−1, with ranges from −22.5 to −17.5 km s−1. The contour levels are 1 Jy beam−1 km s−1 × (1, 5, 10, 20, 40, 80, 200). The thick black contour in the left panel shows the 4σ level of the 7 m continuum emission.

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