Metallicity Mapping of the Ionized Diffuse Gas at the Milky Way Disk–Halo Interface
Metals in the diffuse, ionized gas at the boundary between the Milky Way’s interstellar medium (ISM) and circumgalactic medium, known as the disk–halo interface (DHI), are valuable tracers of the feedback processes that drive the Galactic fountain. However, metallicity measurements in this region ar...
Saved in:
| Main Authors: | Bo-Eun Choi, Jessica K. Werk, Kirill Tchernyshyov, J. Xavier Prochaska, Yong Zheng, Mary E. Putman, Drummond B. Fielding, Jay Strader |
|---|---|
| Format: | Article |
| Language: | English |
| Published: |
IOP Publishing
2024-01-01
|
| Series: | The Astrophysical Journal |
| Subjects: | |
| Online Access: | https://doi.org/10.3847/1538-4357/ad84f8 |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
-
On the Origin of the 107 K Hot Emitting Gas in the Circumgalactic Medium of the Milky Way
by: Mukesh Singh Bisht, et al.
Published: (2024-01-01) -
The Local Stellar Halo is Not Dominated by a Single Radial Merger Event
by: Thomas Donlon II, et al.
Published: (2022-01-01) -
Rising from the Ashes: A Metallicity-dependent Star Formation Gap Splits the Milky Way’s α Sequences
by: Angus Beane
Published: (2025-01-01) -
A New Rarity Assessment of the “Disk of Satellites”: The Milky Way System Is the Exception Rather Than the Rule in the ΛCDM Cosmology
by: Chanoul Seo, et al.
Published: (2024-01-01) -
The Rapid Formation of the Metal-poor Milky Way
by: Turner Woody, et al.
Published: (2025-01-01)