3 papers
astro-ph.GA2026
Simulating winds in the Galactic centre: I. Supernova-driven multiphase outflows and HI cloud acceleration
Nicolas Peschken, Enrico M. Di Teodoro, MichaÅ Hanasz +5
The centre of the Milky Way (MW) hosts powerful multiphase outflows, as evidenced by the Fermi and eROSITA bubbles, and by cold atomic hydrogen (HI) gas clouds detected up to a few…
astro-ph.GA2026
Modelling the non-equilibrium chemistry of the Milky Way's cold nuclear wind
Karlie A. Noon, Mark R. Krumholz, Naomi M. McClure-Griffiths +2
Cold atomic and molecular gas are commonly observed in the winds of both external galaxies and the Milky Way, yet the survival and origin of these cool phases within hot galactic w…
astro-ph.GA2026
Modeling the Milky Way wind: Supernova-driven outflows accelerate HI clouds near the Galactic center
Andrea Afruni, Enrico M. Di Teodoro, Lucia Armillotta +2
Multiwavelength observations, from radio to X-rays, have revealed the presence of multiphase high-velocity gas near the center of the Milky Way likely associated with powerful gala…