The H I halo in the inner galaxy
Abstract
There is 21 cm emission from corotating H I in the inner Galaxy to |z| ≥ 1000 pc from the plane. Over most of the inner Galaxy more than 10% of the H I emission at the subcentral points comes from |z| > 500 pc. High-z H I is not present ⪉3 kpc from the galactic center, but appears suddenly near R = 3.5 kpc, in qualitative agreement with Bregman's model for a wind from the bulge. The scale height and surface density of the halo are approximately constant over 4 ≤ R ≤ 8 kpc. In this region nH(z) has a long exponential tail with a scale height ≡500 pc and a density of 0.012 cm-3 at |z| = 750 pc.
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The H i layer of the Galactic disk is much thinner at Galactocentric radius R ≲ 3 kpc.
“The author found that the H i layer of the Galactic disk is much thinner at Galactocentric radius, R ≲ 3 kpc.”
From The Fermi/eROSITA bubbles: a look into the nuclear outflow from the Milky Way (2024) · cites this paper as Lockman 1984
The H i scale height drops sharply by almost a factor of 3-4 as one goes toward the Galactic Center.
“The H i scale height was found to drop sharply by almost a factor of 3 -4 as one goes toward the GC.”
From The Fermi/eROSITA bubbles: a look into the nuclear outflow from the Milky Way (2024) · cites this paper as Lockman 1984
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Fujimoto, Y., Bryan, G. L., Tasker, E. J., Habe, A., & Simpson, C. M. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw1461 · Cited by 17 · see citing works
Interaction of the galactic-centre super bubbles with the gaseous disc
Sofue, Y., & Kataoka, J. (2021) · Monthly notices of the Royal Astronomical Society · doi:10.1093/mnras/stab1857 · Cited by 11 · see citing works
The Cool Phase of the Interstellar Medium: Atomic Gas
Brinks, E. (1990) · Astrophysics and space science library · doi:10.1007/978-94-009-0595-5_3 · Cited by 17 · see citing works
Superbubble evolution in disk galaxies, I. Study of blow-out by analytical modelsPreprint
Baumgartner, V., & Breitschwerdt, D. (2014) · arXiv (Cornell University) · doi:10.48550/arxiv.1402.0194 · Cited by 19 · see citing works
The Effects of Cosmic-Ray Diffusion and Radiative Cooling on the Galactic Wind of the Milky Way
Shimoda, J., & Inutsuka, S. (2022) · The Astrophysical Journal · doi:10.3847/1538-4357/ac4110 · Cited by 16 · see citing works
The 'Carina Flare' supershell: probing the atomic and molecular ISM in a galactic chimneyPreprint
Dawson, J. R., Mizuno, N., Onishi, T., McClure‐Griffiths, N. M., & Fukui, Y. (2008) · Cited by 16 · see citing works
Turbulence in interstellar clouds
Falgarone, E. G. (2007) · Springer eBooks · doi:10.1007/bfb0114842 · Cited by 16 · see citing works
Giant H i hole inside the 3 kpc ring and the North Polar Spur—The Galactic crater
Sofue, Y. (2017) · Publications of the Astronomical Society of Japan · doi:10.1093/pasj/psx067 · Cited by 15 · see citing works
- Authors
- Lockman, F. J.
- Corresponding author
- Lockman, F. J.
- ORCID
- Lockman, F. J.
- Venue
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Published
- 1984-08
- Volume
- 283
- Pages
- 90
- ISSN
- 0004-637X (ISSN-L)
- 1538-4357
- OpenAlex
- W2089132604
- Cited by
- 200
- References
- 0
- Citations by year
- 2026: 3 · 2025: 1 · 2024: 4 · 2023: 4 · 2022: 7 · 2021: 7 · 2020: 6 · 2019: 7 · 2018: 5 · 2017: 4 · 2016: 7 · 2015: 8 · 2014: 2 · 2013: 7 · 2012: 5
- FWCI
- 6.47
- Type
- journal article
- Language
- en
- Open access
- closed
- Locations
- The Astrophysical Journal (publishedVersion)
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astrophysics and Star Formation Studies
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Galaxies: Formation, Evolution, Phenomena
- Keywords
- HI halo, inner Milky Way, HI 21 cm emission, scale height, exponential density profile, Galactic disk
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