UvA-DARE (Digital Academic Constraints on particle acceleration in SS433/W50 from MAGIC and H.E.S.S. observations
UvA-DARE (Digital Academic Constraints on particle acceleration in SS433/W50 from MAGIC and H.E.S.S. observations
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UvA-DARE（来自 MAGIC 和 H.E.S.S. 观测的 SS433/W50 中粒子加速的数字学术约束
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通讯作者：
H. Cooper
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作者：
R. Parry;W. Li;H. Cooper
上下文。在微类星体SS433中发生的大喷流动能和非热过程使该源非常适合作为超高能(VHE)伽马射线发射器。对于中心X射线双星系统和SS433喷流与周围W50星云的相互作用区域，都预测了高于当前切伦科夫望远镜灵敏度极限的伽马射线fl。以前已经报道过在较低能量下的非热发射，这表明系统中正在发生明显的ffi粒子加速。我们探索了这些相互作用区的衰减量(和恒星周围的中心双星flu)。
Context. The large jet kinetic power and non-thermal processes occurring in the microquasar SS 433 make this source a good candidate for a very high-energy (VHE) gamma-ray emitter. Gamma-ray fluxes above the sensitivity limits of current Cherenkov telescopes have been predicted for both the central X-ray binary system and the interaction regions of SS 433 jets with the surrounding W50 nebula. Non-thermal emission at lower energies has been previously reported, indicating that e ffi cient particle acceleration is taking place in the system. We explore the attenuation ( and circumstellar central binary fluxes in these interaction regions.