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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 1.

Integrated intensity map of the 13CS 5–4 transition with colored scale, shown as a bar above the figure. The boundary contour in black is for the 0.15 Jy beam−1 km s−1 intensity, and the white contours are for the 0.15 × [3, 5, 7] Jy beam−1 km s−1 intensities. The magenta contour lines show the H30α line with a scale of 0.5 × [1, 2, 3, 4, 5] Jy beam−1 km s−1. The labels A1–A13 are the positions of the dust continuum peaks identified by Liu et al. (2015). The beam of 0.″75 × 0.″60 (﹩\mathrm{PA}=88^\circ ﹩) is shown in the bottom left corner.

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