QR-Code

Revision of the γ-Ray Emission from SNR CTB 109 with the Fermi Large Area Telescope

CTB 109 is a middle-aged shell-type supernova remnant (SNR) with bright thermal X-ray emission. We reanalyze the GeV γ -ray emission from CTB 109 using 13 yr of Pass 8 data recorded by the Fermi Large Area Telescope. The γ -ray emission of CTB 109 shows a center bright morphology, which is well cons...

Ausführliche Beschreibung

Gespeichert in:
Bibliografische Detailangaben
Hauptverfasser: Yuliang Xin, Qizhen Zhao, Xiaolei Guo
Format: Artigo
Sprache:Inglês
Veröffentlicht: IOP Publishing 2023-01-01
Schriftenreihe:The Astrophysical Journal
Schlagworte:
Online-Zugang:https://doi.org/10.3847/1538-4357/acac89
Tags: Tag hinzufügen
Keine Tags, Fügen Sie das erste Tag hinzu!