The Nature of γ-Ray Emission from HESS J1912+101

Since the discovery of HESS J1912+101 at teraelectronvolt energies, its nature has been extensively studied. Due to the absence of X-ray and radio counterparts, whether its γ -ray emission is produced by relativistic electrons or ions is still a matter of debate. We reanalyze its megaelectronvolt to...

وصف كامل

التفاصيل البيبلوغرافية
الحاوية / القاعدة:	The Astrophysical Journal
المؤلفون الرئيسيون:	Yuan Li, Siming Liu, Yu He
التنسيق:	مقال
اللغة:	الإنجليزية
منشور في:	IOP Publishing 2023-01-01
الموضوعات:	Supernova remnants Molecular clouds High energy astrophysics
الوصول للمادة أونلاين:	https://doi.org/10.3847/1538-4357/ace344

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