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...

全面介紹

書目詳細資料

Principais autores:	Yuliang Xin, Jian Tang, Weixiong Ding, Xi Liu, Yunfeng Zhang, Xiaolei Guo
格式:	Artigo
語言:	Inglês
出版:	IOP Publishing 2025-01-01
叢編:	The Astrophysical Journal
主題:	Supernova remnants Gamma-ray sources Pulsar wind nebulae
在線閱讀:	https://doi.org/10.3847/1538-4357/adb282
標簽:	添加標簽 沒有標簽, 成為第一個標記此記錄!