Abstract
We make a comprehensive study of H I absorption toward H II regions located within |l| < 10°. Structures in the extreme inner Galaxy are traced using the longitude-velocity space distribution of this absorption. We find significant H I absorption associated with the Near and Far 3 kpc Arms, the Connecting Arm, Bania's Clump 1, and the H I Tilted Disk. We also constrain the line-of-sight distances to H II regions, by using H I absorption spectra together with the H II region velocities measured by radio recombination lines.
Original language | English |
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Article number | 117 |
Pages (from-to) | 1-18 |
Number of pages | 18 |
Journal | Astrophysical Journal |
Volume | 774 |
Issue number | 2 |
DOIs | |
Publication status | Published - 10 Sept 2013 |
Externally published | Yes |
Bibliographical note
Copyright 2013 The American Astronomical Society. First published in the Astrophysical Journal, 774(2), 117, 2013. The original publication is available at https://doi.org/10.1088/0004-637X/774/2/117, published by IOP Publishing. Version archived for private and non-commercial use with the permission of the author/s and according to publisher conditions. For further rights please contact the publisher.Keywords
- Galaxy: structure
- Hii regions