3D MC. I. X-Ray Tomography Begins to Unravel the 3D Structure of a Molecular Cloud in our Galaxy’s Center
Astronomers have used observations of the Galactic gas and dust via infrared, microwave, and radio to study molecular clouds in extreme environments such as the Galactic center. More recently, X-ray telescopes have opened up a new wavelength range in which to study these molecular clouds. Previous f...
Saved in:
| Main Authors: | Samantha W. Brunker, Cara Battersby, Danya Alboslani, Maïca Clavel, Daniel L. Walker, Dani Lipman, H Perry Hatchfield, Régis Terrier |
|---|---|
| Format: | Article |
| Language: | English |
| Published: |
IOP Publishing
2025-01-01
|
| Series: | The Astrophysical Journal Letters |
| Subjects: | |
| Online Access: | https://doi.org/10.3847/2041-8213/adba5e |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
-
3D MC. II. X-Ray Echoes Reveal a Clumpy Molecular Cloud in the CMZ
by: Danya Alboslani, et al.
Published: (2025-01-01) -
Red Stellar Populations and Dust Extinction toward W3
by: J. L. Campbell, et al.
Published: (2025-01-01) -
3D CMZ. I. Central Molecular Zone Overview
by: Cara Battersby, et al.
Published: (2025-01-01) -
Spatially Resolved Galaxy–Dust Modeling with Coupled Data-driven Priors
by: Jared C. Siegel, et al.
Published: (2025-01-01) -
Fuzzy Galaxies or Cirrus? Decomposition of Galactic Cirrus in Deep Wide-field Images
by: Qing Liu, et al.
Published: (2025-01-01)