Abstract
I consider several aspects of the Galactic HI distribution, kinematics, and morphology at R < R 0, in particular; the rotation curve of the inner few kpc; the variation of HI across the inner disks of the Milky Way and other galaxies; the amount of HI inferred in the disk (with implications for the CO-H2 conversion factor); and lastly, the physical disposition of neutral atomic gas and some consequences of the required structure of HI ‘clouds’ for optical and uv absorption-line profile analysis.
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Liszt, H.S. (1992). HI in the Inner Galaxy. In: Blitz, L. (eds) The Center, Bulge, and Disk of the Milky Way. Astrophysics and Space Science Library, vol 180. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-2813-1_6
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DOI: https://doi.org/10.1007/978-94-011-2813-1_6
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