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Searching for Connections among the Fermi Bubbles, the Galactic Center GeV Excess, and Loop I

Special Issue Information

Dear Colleagues,

The Fermi bubbles, the Galactic center excess, and Loop I are bright extended sources of gamma rays. In spite of a significant effort to explain the origin of these objects, many unresolved questions remain. In this Special Issue we will review recent data analysis and theoretical modeling to search for possible connections among the three “elephants” in the gamma-ray sky. We will also discuss how future observations can shed light on the origin of these features.

Dr. Dmitry Malyshev
Guest Editor

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Submitted manuscripts should not have been published previously, nor be under consideration for publication elsewhere (except conference proceedings papers). All manuscripts are thoroughly refereed through a single-blind peer-review process. A guide for authors and other relevant information for submission of manuscripts is available on the Instructions for Authors page. Galaxies is an international peer-reviewed open access semimonthly journal published by MDPI.

Please visit the Instructions for Authors page before submitting a manuscript. The Article Processing Charge (APC) for publication in this open access journal is 1400 CHF (Swiss Francs). Submitted papers should be well formatted and use good English. Authors may use MDPI's English editing service prior to publication or during author revisions.

Keywords

  • Milky Way
  • Galactic Center and Halo
  • Cosmic Rays
  • Gamma Rays
  • Dark Matter
  • Diffuse Emission and Point Sources in the Galactic Halo

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Galaxies - ISSN 2075-4434