Issue |
EPJ Web Conf.
Volume 136, 2017
RICAP16, 6th Roma International Conference on Astroparticle Physics
|
|
---|---|---|
Article Number | 03011 | |
Number of page(s) | 4 | |
Section | Gamma Rays | |
DOI | https://doi.org/10.1051/epjconf/201713603011 | |
Published online | 23 March 2017 |
https://doi.org/10.1051/epjconf/201713603011
Fermi Bubbles: an elephant in the gamma-ray sky
Erlangen Centre for Astroparticle Physics, Erwin-Rommel-Str. 1, D-91058 Erlangen, Germany
a e-mail: dmitry.malyshev@fau.de
Published online: 23 March 2017
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.
© The Authors, published by EDP Sciences, 2017
This is an Open Access article distributed under the terms of the Creative Commons Attribution License 4.0, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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