A periodic gamma-ray signal detected from the micro-quasar SS 433 cannot be associated with its jet. Instead, a new mechanism capable of channelling most of SS 433’s kinetic power to large distances is needed to explain the observations.

中文翻译：

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来自SS 433的伽马射线回波

从微类星体433检测到的周期性伽马射线信号无法与其喷射相关联。取而代之的是，需要一种能够将SS 433的大部分动能引导至远距离的新机制，以解释这些发现。