Challenges in explaining the Galactic Center gamma-ray excess with millisecond pulsars
Challenges in explaining the Galactic Center gamma-ray excess with millisecond pulsars
Millisecond pulsars have been discussed as a possible source of the gamma-ray excess observed from the region surrounding the Galactic Center. With this in mind, we use the observed population of bright low-mass X-ray binaries to estimate the number of millisecond pulsars in the Inner Galaxy. This calculation suggests that …