Spectrum and Morphology of the Very-high-energy Source HAWC J2019+368
نویسندگان
چکیده
Abstract The MGRO J2019+37 region is one of the brightest sources in sky at TeV energies. It was detected second HAWC catalog as 2HWC J2019+367 and here we present a detailed study this using data from HAWC. This analysis resolves into two sources: J2019+368 J2016+371. We associate J2016+371 with evolved supernova remnant CTB 87, although its low significance prevents time. An investigation morphology (including possible energy-dependent morphology) spectrum for focus work. PSR J2021+3651 X-ray pulsar wind nebula, Dragonfly nebula. Modeling measured by Suzaku reveals ?7 kyr nebula system producing observed emission ? -ray
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ژورنال
عنوان ژورنال: The Astrophysical Journal
سال: 2021
ISSN: ['2041-8213', '2041-8205']
DOI: https://doi.org/10.3847/1538-4357/abecda