HAWC and Fermi-LAT detection of extended emission from the unidentified source 2HWC J2006+341
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Authors
Albert, Andrea
Alfaro Molina, José Rubén
Álvarez Ochoa, César
Ángeles Camacho, José Roberto
Araya Arguedas, Miguel
Arteaga Velázquez, Juan Carlos
Arun Babu, Kollamparambil Paul
Ávila Rojas, Daniel Omar
Ayala Solares, Hugo Alberto
Baghmanyan, Vardan
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Abstract
The discovery of the TeV point source 2HWC J2006+341 was reported in the second HAWC gamma-ray catalog. We present a follow-up study of this source here. The TeV emission is best described by an extended source with a soft spectrum. At GeV energies, an extended source is significantly detected in Fermi-LAT data. The matching locations, sizes, and spectra suggest that both gamma-ray detections correspond to the same source. Different scenarios for the origin of the emission are considered and we rule out an association to the pulsar PSR J2004+3429 due to extreme energetics required, if located at a distance of 10.8 kpc.
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PHYSICS, ULTRAVIOLET RADIATION, GAMMA RAYS, INTERSTELLAR MEDIUM
Citation
https://iopscience.iop.org/article/10.3847/2041-8213/abbfae