Figure 2 from Where is OH and Does It Trace the Dark Molecular Gas (DMG)?

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Where is OH and Does It Trace the Dark Molecular Gas (DMG)?

Authors: Di Li, Ningyu Tang, Hiep Nguyen, J. R. Dawson, Carl Heiles, Duo Xu, Zhichen Pan, c Paul F. Goldsmith, Steven J. Gibson, Claire E. Murray, Tim Robishaw, N. M. McClure-Griffiths, John Dickey, Jorge Pineda, Snežana Stanimirović, L. Bronfman, and Thomas Troland

2018 The Astrophysical Journal Supplement Series 235 1.

Provider: AAS Journals

Caption: Figure 2.

Illustration of derived parameters from the fits to the absorption (upper panel) and expected emission (lower panel) profiles for the source P0428+20. The thin solid lines show the data ; the thick solid lines are the fits. The solid lines below the dashed lines present the residuals for absorption and fitted expected emission, respectively.

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