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High energy emission from the center of our Galaxy

Date

Authors

Chernyakova, M

Malyshev, D

Aharonian, F

Crocker, Roland

Jones, David I

Publisher

Proceedings of Science

Abstract

Employing data collected during the first 25 months observations by the Fermi-LAT, we describe and subsequently seek to model the very-high energy (> 300 MeV) emission from the central few parsecs of our Galaxy. Using the combination of Fermi data on 1FGL

Keywords

Keywords: Angular resolution; Gamma ray sources; Gamma ray telescope; High energy emission; Morphological information; Parameter choice; Radio continuum; Spectral region; Galaxies; Protons; Tellurium compounds; Gamma rays

URI

http://hdl.handle.net/1885/83741

Collections

ANU Research Publications

Source

Proceedings of Science

Type

Conference paper

Restricted until

2037-12-31

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