Galactic binaries can explain the Fermi Galactic centre excess and 511 keV emission
Author:
Affiliation:
1. GRAPPA, Institute for Theoretical Physics and Delta Institute for Theoretical Physics, University of Amsterdam, Science Park 904, NL-1098XH Amsterdam, The Netherlands
2. University Grenoble Alpes, USMB, CNRS, LAPTh, F-74940 Annecy, France
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/480/3/3826/25520223/sty2135.pdf
Reference160 articles.
1. The consistency of Fermi-LAT observations of the galactic center with a millisecond pulsar population in the central stellar cluster
2. FERMI LARGE AREA TELESCOPE THIRD SOURCE CATALOG
3. FERMI-LAT OBSERVATIONS OF HIGH-ENERGYγ-RAY EMISSION TOWARD THE GALACTIC CENTER
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