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Expanding Molecular Shell and Possible γ-ray Source Associated with Supernova Remnant Kesteven 67

Fuente: arXiv

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Dettagli Bibliografici
Autori principali:	Shen, Yun-Zhi, Chen, Yang, Zhang, Xiao, Tu, Tian-Yu, Zhong, Wen-Juan, Zhang, Qian-Qian, Liu, Qian-Cheng
Natura:	Preprint
Pubblicazione:	2025
Soggetti:	High Energy Astrophysical Phenomena
Accesso online:	Acceder al recurso
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