The role of magnetic fields in shaping $γ$-ray emission from the Fermi bubbles

Documenti analoghi

• Contribution of the Cygnus bubble to the Galactic cosmic ray spectrum and diffuse $γ$-ray emissions
  di: Nie, Lin, et al.
  Pubblicazione: (2024)
• Hydrodynamic model of nonthermal emission from the Fermi bubbles
  di: Dogiel, V. A., et al.
  Pubblicazione: (2026)
• Detection of polarized Fermi-bubble synchrotron and dust emission
  di: Keshet, Uri
  Pubblicazione: (2024)
• Detection of the extended $γ$-ray emission from the new supernova remnant G321.3-3.9 with Fermi-LAT
  di: Guo, Xiaolei, et al.
  Pubblicazione: (2024)
• Likely detection of GeV γ-ray emission from pulsar wind nebula G32.64+0.53 with Fermi-LAT
  di: Xiao, Yifan, et al.
  Pubblicazione: (2024)