# HAWC Study of the Ultra-high-energy Spectrum of MGRO J1908+06

HAWC Collaboration

Resultado de la investigación: Contribución a una revistaArtículorevisión exhaustiva

## Resumen

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.

Idioma original Inglés 116 Astrophysical Journal 928 2 https://doi.org/10.3847/1538-4357/ac56e5 Publicada - 1 abr 2022

## Huella

Profundice en los temas de investigación de 'HAWC Study of the Ultra-high-energy Spectrum of MGRO J1908+06'. En conjunto forman una huella única.