Figure 3 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 3.

Same as Figure 2. Starting from the top-left panel to the right and from top to bottom: the central source component becomes less and less prominent. Some transitions do not display a central dominating component at all, like the ones in the two bottom rows.

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