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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 10.

Left panel: ratio between the zero moment of the CH3OH ﹩({{\rm{E}}}_{2})\,\,{J}_{{K}_{a}{K}_{c}}={5}_{-\mathrm{1,0}}\to {4}_{\mathrm{0,0}}﹩ and (E1) ﹩{2}_{\mathrm{1,1}}\to {1}_{\mathrm{1,0}}﹩ lines. Right panel: zero moment of the CH3OH ﹩({{\rm{E}}}_{2})\,\,{J}_{{K}_{a}{K}_{c}}={5}_{-\mathrm{1,0}}\to {4}_{\mathrm{0,0}}﹩ emission. The three masers (yellow circles) correspond to the three strongest sources (whose coordinates are given in Table 2), conspicuous even in the logarithmic color stretch. Red crosses and numbers show continuum 3 mm sources near the masers.

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