Several X-ray binaries (XRBs) have been identified to be associated with supernova remnants (SNRs). Because of the short lifetimes of SNRs, this leaves them to be the youngest known XRBs. This small group of binaries provides valuable information on the formation of compact stars under the framework of massive binary evolution. In this paper we review the observational characteristics of these youngest XRBs and discuss their possible implications on the initial conditions of compact stars and their interaction with the companion stars.

中文翻译：

---

最年轻的 X 射线双星

一些 X 射线双星 (XRB) 已被确定与超新星遗迹 (SNR) 相关。由于 SNR 的寿命很短，这使得它们成为已知的最年轻的 XRB。这一小群双星提供了在大规模双星演化框架下致密恒星形成的宝贵信息。在本文中，我们回顾了这些最年轻的 XRB 的观测特征，并讨论了它们对致密星初始条件及其与伴星相互作用的可能影响。