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Date and Time of the Query: 2019-08-21 T10:56:50 PDT
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For refcode 2003ApJ...586..230R:
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2003ApJ...586..230R A Far Ultraviolet Spectroscopic Explorer Survey of Molecular Hydrogen in Intermediate-Velocity Clouds in the Milky Way Halo Philipp Richter, Bart P. Wakker, Blair D. Savage, and Kenneth R. Sembach Abstract. Far Ultraviolet Spectroscopic Explorer (FUSE) data are used to investigate the molecular hydrogen (H_2_) content of intermediate-velocity clouds (IVCs) in the lower halo of the Milky Way. We analyze interstellar absorption toward 56 (mostly extragalactic) background sources to study H_2_ absorption in the Lyman and Werner bands in 61 IVC components at H I column densities >= 10^19^ cm^-2^. For data with good signal-to-noise ratio (S/N) (~9 per resolution element and higher), H_2_ in IVC gas is convincingly detected in 14 cases at column densities varying between ~10^14^ and ~10^17^ cm^-2^. We find an additional 17 possible H_2_ detections in IVCs in FUSE spectra with lower S/N. The molecular hydrogen fractions, f, vary between 10^-6^ and 10^-3^, implying a dense, mostly neutral gas phase that is probably related to the cold neutral medium (CNM) in these clouds. If the H_2_ stays in formation-dissociation equilibrium, the CNM in these clouds can be characterized by compact (D~0.1 pc) filaments with volume densities on the order of n_H_~30 cm^-3^. The relatively high detection rate of H_2_ in IVC gas implies that the CNM in these clouds is ubiquitous. More dense regions with much higher molecular fractions may exist, but it would be difficult to detect them in absorption because of their small size. Keywords: Galaxy: Halo, ISM: Abundances, ISM: Clouds, Galaxies: Quasars: Absorption Lines, Ultraviolet: ISM
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