Figure 13 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 13.

Each curve shows the minimum column density necessary to produce a Gaussian line peak of 5σ ≈ 0.3 K and FWHM = 4 km s⁻¹ in at least one transition in our spectral coverage vs. the excitation temperature (assuming LTE).

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