Strong Support for the Millisecond Pulsar Origin of the Galactic Center GeV Excess

Using γ-ray data from the Fermi Large Area Telescope, various groups have identified a clear excess emission in the Inner Galaxy, at energies around a few GeV. This excess resembles remarkably well a signal from dark-matter annihilation. One of the most compelling astrophysical interpretations is th...

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Veröffentlicht in:Physical review letters 2016-02, Vol.116 (5), p.051102-051102, Article 051102
Hauptverfasser: Bartels, Richard, Krishnamurthy, Suraj, Weniger, Christoph
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Sprache:eng
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