Figure 10 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 10.

Representative spectra as described in Section 4.3. The 3C192 sightline has only H I seen in absorption. One component of the 3C133 sightline has OH and H I in absorption and CO and its isotopologues in emission. The 3C132 sightline has one gas component with both OH and H I, but no detectable CO transitions.

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