Figure 12 from Chemistry of the High-mass Protostellar Molecular Clump IRAS 16562

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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 12.

Propyne (CH₃CCH) physical parameters toward IRAS 16562−3959. The left and right panels show the column density and excitation temperature, respectively. We show in each panel the location of the NW cloud, the N-red cloud, the NEC-wall, the Diffuse Ridge, the position of DR (a), (b), and (c) (black crosses), and continuum sources 8 and 10 (red crosses).

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