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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 9.

Example of the spectral line fitting for G286c5. Here we use one Gaussian component to fit the spectra of ﹩{{\rm{N}}}_{2}{{\rm{D}}}^{+}﹩(3–2), ﹩{\mathrm{DCO}}^{+}﹩(3–2), and ﹩\mathrm{DCN}﹩(3–2) and two components for C18O(2–1).

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