Fermi Bubbles: an Elephant in the Gamma-ray Sky
arXiv:1704.02629 · doi:10.1051/epjconf/201713603011
Abstract
The Fermi bubbles are one of the most remarkable features in the gamma-ray sky revealed by the Fermi Large Area Telescope (LAT). The nature of the gamma-ray emission and the origin of the bubbles are still open questions. In this note, we will review some basic features of leptonic and hadronic modes of gamma-ray production. At the moment, gamma rays are our best method to study the bubbles, but in order to resolve the origin of the bubbles multi-wavelength and multi-messenger observations will be crucial.
Published in proceedings for RICAP16 conference
References in corpus (8)
- Giant Gamma-ray Bubbles from Fermi-LAT: AGN Activity or Bipolar Galactic Wind?
- The Two Young Star Disks in the Central Parsec of the Galaxy: Properties, Dynamics and Formation
- The Spectrum and Morphology of the Fermi Bubbles
- Fermi Gamma-ray Imaging of a Radio Galaxy
- The Fermi Bubbles: Giant, Multi-Billion-Year-Old Reservoirs of Galactic Center Cosmic Rays
- Suzaku observations of the diffuse x-ray emission across the fermi bubbles' edges
- Probing the Fermi Bubbles in Ultraviolet Absorption: A Spectroscopic Signature of the Milky Way's Biconical Nuclear Outflow
- Fossil imprint of a powerful flare at the Galactic Centre along the Magellanic Stream