Speaker
Joshua Wood
(University of Maryland, College Park)
Description
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.
Registration number following "ICRC2015-I/" | 1160 |
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Collaboration | HAWC |
Author
Brian Baughman
(University of Maryland, College Park)
Co-authors
Mr
Hugo Alberto Ayala Solares
(Michigan Technological University)
Joshua Wood
(University of Maryland, College Park)