%0 Journal Article
%T HAWC Study of the Ultra-high-energy Spectrum of MGRO J1908+06
%A HAWC Collaboration (Albert, A. et al
%A Salesa Greus, F.
%J Astrophysical Journal
%D 2022
%V 928
%N 2
%I IOP Publishing Ltd
%@ 0004-637x
%G English
%F HAWCCollaborationAlbert+SalesaGreus2022
%O WOS:000776453700001
%O exported from refbase (https://references.ific.uv.es/refbase/show.php?record=5187), last updated on Sat, 16 Apr 2022 19:21:00 +0000
%X We report TeV gamma-ray observations of the ultra-high-energy source MGRO J1908+06 using data from the High Altitude Water Cherenkov Observatory. This source is one of the highest-energy known gamma-ray sources, with emission extending past 200 TeV. Modeling suggests that the bulk of the TeV gamma-ray emission is leptonic in nature, driven by the energetic radio-faint pulsar PSR J1907+0602. Depending on what assumptions are included in the model, a hadronic component may also be allowed. Using the results of the modeling, we discuss implications for detection prospects by multi-messenger campaigns.
%R 10.3847/1538-4357/ac56e5
%U https://arxiv.org/abs/2112.00674
%U https://doi.org/10.3847/1538-4357/ac56e5
%P 116-13pp