Strong Support for the Millisecond Pulsar Origin of the Galactic Center GeV Excess
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 that the excess is caused …