Study of the source HAWC J0615+2213 in the IC 443 region
ORAL
Abstract
After studying the supernova remnant IC 443 with HAWC data, we found an extended component in the region, with no clear low-energy counterparts. A molecular cloud interpretation was tested but found insufficient to explain the full extent of the emission. An alternative explanation is that the signal originates from a TeV halo associated with PSR B0611+22, which is surrounded by the extended emission and exhibits properties consistent with a TeV Halo. We report on the analysis and results of the halo hypothesis.
*US National Science Foundation (NSF); the US Department of Energy Office of High-Energy Physics; the Laboratory Directed Research and Development (LDRD) program of Los Alamos National Laboratory; Consejo Nacional de Ciencia y Tecnologia (CONACyT), Mexico
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Presenters
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Hugo Ayala
- Temple University