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The GeV γ-Ray Emission from the Composite Supernova Remnant CTB 87

We report the GeV γ -ray emission around the composite supernova remnant (SNR) CTB 87 with more than 16 yr of PASS 8 data recorded by the Fermi Large Area Telescope. Two separate point sources with different GeV spectra are identified in this region: one has a soft γ -ray spectrum, likely due to int...

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Principais autores: Yuliang Xin, Jian Tang, Weixiong Ding, Xi Liu, Yunfeng Zhang, Xiaolei Guo
Formato: Artigo
Idioma:Inglês
Publicado: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
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Acceso en liña:https://doi.org/10.3847/1538-4357/adb282
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