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 Series23645.
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).