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CHEMICAL DIAGNOSTICS OF THE MASSIVE STAR CLUSTER-FORMING CLOUD G33.92+0.11. I. 13CS, CH3OH, CH3N, OCS, H2S, SO2, and SiO

  • Authors: Young Chol Minh, Hauyu Baobab Liu, and Roberto Galvań-Madrid

2016 The Astrophysical Journal 824 99.

  • Provider: AAS Journals

Caption: Figure 4.

Observed spectra of the CH3CN 12–11 line toward the peak emission position of the A1 clump. The red line is the Gaussian fit results, and the residuals are shown right below the spectrum. The CH﹩{}_{3}^{\;13}﹩CN 12–11 spectrum is also shown in blue. Rotational diagrams of the K-components of the CH3CN 12–11 line toward the A1, A2, and A5 peaks. Errors are 3σ of the observed uncertainties. Rotational temperatures are indicated for the A1 results.

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