One-kpc Expanding Cylinder of HI-Gas around the Galactic Center
arXiv:2205.02078 · doi:10.1093/pasj/psac034
Abstract
We report the discovery of an expanding cylinder of HI gas of radius 1 kpc and vertical extent 800 pc by analyzing the 21-cm line survey data from the literature. The cylinder is expanding at 150 km s and rotating at 100 km s, and is interpreted as due to a high-velocity conical wind at km s from the Galactic Center. The total mass of the cylinder is estimated to be and kinetic energy ergs.
Accepted for PASJ Letters. 4 pages 3 figures
References in corpus (9)
- HI4PI: A full-sky HI survey based on EBHIS and GASS
- Giant Gamma-ray Bubbles from Fermi-LAT: AGN Activity or Bipolar Galactic Wind?
- Gas flow models in the Milky Way embedded bars
- Observation of Acceleration of HI Clouds Within the Fermi Bubbles
- Recognizing the fingerprints of the Galactic bar: a quantitative approach to comparing model (l,v) distributions to observation
- The 200-pc Molecular Cylinder in the Galactic Centre
- Interaction of the Galactic-Centre Super Bubbles with the Gaseous Disc
- Giant HI Hole inside the 3-kpc Ring and the North Polar Spur - The Galactic Crater -
- Diagnostics of Gaseous Halo of the Milky Way by a Shock Wave from the Galactic Centre