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Chemistry of the High-mass Protostellar Molecular Clump IRAS 16562–3959

  • Authors: Andrés E. Guzmán, Viviana V. Guzmán, Guido Garay, Leonardo Bronfman, and Federico Hechenleitner

2018 The Astrophysical Journal Supplement Series 236 45.

  • Provider: AAS Journals

Caption: Figure 14.

Left panel: moment zero quotient between the H13CN and HC15N ﹩J=0\to 1﹩ transitions. Right panel: moment zero quotient between the H13CN and HN13C ﹩J=0\to 1﹩ transitions. Blue contours are drawn at the 25%, 50%, and 75% of the peak H13CN moment zero emission. Cyan contours correspond to NH2D emission as in Figure 15. In both panels, we indicate the N-red, NW- and Diffuse Ridge markers as in Figure 7.

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