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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 7.

Optical depth ratio (R67/65 = τ1667/τ1665) as a function of excitation temperature difference (Tex(1667) − Tex(1665)) for the 1667 and 1665 MHz OH lines. The horizontal and vertical dashed lines indicate 1.8 and 0.0, the values for LTE excitation. The error bars indicate the 1σ formal uncertainties propagated through from the Gaussian fits. The black points are those consistent with LTE to within the 1σ errors; the red points are inconsistent. The vertical shaded region represents ﹩| {\rm{\Delta }}{T}_{\mathrm{ex}}| \lt 2\,{\rm{K}}﹩.

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