  Measurements of the nearby pulsars Geminga and B0656+14 by the HAWC and
Milagro telescopes have revealed the presence of bright TeV-emitting halos
surrounding these objects. If young and middle-aged pulsars near the Galactic
Center transfer a similar fraction of their energy into TeV photons, then these
sources could plausibly dominate the emission that is observed by HESS and
other ground-based telescopes from the innermost $\sim$$10^2$ parsecs of the
Milky Way. In particular, both the spectral shape and the angular extent of
this emission is consistent with TeV halos produced by a population of pulsars,
although the reported correlation of this emission with the distribution of
molecular gas suggests that diffuse hadronic processes also must contribute.
The overall flux of this emission requires a birth rate of ~100-1000 neutron
stars per Myr near the Galactic Center, in good agreement with recent
estimates.
