Geminga is a radio-quiet pulsar ~250 parsecs from Earth that was first discovered as a GeV gamma-ray source and then identified as a pulsar. Milagro observed an extended TeV source spatially consistent with Geminga. HAWC observes a similarly extended source. Observations of Geminga's flux and extension will be presented.
@article{arxiv.1508.03497,
title = {TeV Gamma-Ray Emission Observed from Geminga with HAWC},
author = {B. M. Baughman and J. Wood},
journal= {arXiv preprint arXiv:1508.03497},
year = {2019}
}
Comments
Presented at the 34th International Cosmic Ray Conference (ICRC2015), The Hague, The Netherlands. See arXiv:1508.03327 for all HAWC contributions