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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מידע ביבליוגרפי

Principais autores:	Yuliang Xin, Jian Tang, Weixiong Ding, Xi Liu, Yunfeng Zhang, Xiaolei Guo
פורמט:	Artigo
שפה:	Inglês
יצא לאור:	IOP Publishing 2025-01-01
סדרה:	The Astrophysical Journal
נושאים:	Supernova remnants Gamma-ray sources Pulsar wind nebulae
גישה מקוונת:	https://doi.org/10.3847/1538-4357/adb282
תגים:	הוספת תג אין תגיות, היה/י הראשונ/ה לתייג את הרשומה!