Simulating the Peculiar Periphery of the Cygnus Loop

The middle-aged Galactic supernova remnant (SNR)- the Cygnus Loop (CL)- displays a peculiar morphology in X-rays, featuring a blowout in the southern region. The underlying process accounting for the formation of the peculiar periphery remains a mystery. To this end, we conduct hydrodynamical simula...

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Veröffentlicht in:	Research in astronomy and astrophysics 2024-12, Vol.24 (12), p.125018
Hauptverfasser:	Shen, Jun-Yu, Bao, Bi-Wen, Zhang, Li
Format:	Artikel
Sprache:	eng
Schlagworte:	Blowouts hydrodynamics ISM: supernova remnants methods: numerical Morphology Parameter modification Parameter sensitivity Red giant stars Simulation Stellar models Stellar winds Supergiant stars Supernova Supernova remnants X-ray astronomy
Online-Zugang:	Volltext
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