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H.E.S.S Observations of the Microquasars Cir X-1, Cyg X-1 and 4U 1755-33

机译:H.E.S.SSSARSARSARS CIR X-1,CYG X-1和4U 1755-33的观察

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A number of microquasars exhibit parsec-scale jets, which in some cases are known to interact with the interstellar medium(ISM). A famous example is the SS-433 system. Here, we summarise H.E.S.S. observations of three further examples in thiscategory with arc-minute scale jets and/or jet/ISM interaction features. The small line-of-sight angle in the Cir X-1 jet makesthis source a potential 'microblazar'. An arc-minute bow-shock radio feature has been blown out by the Cyg X-1 jet, andthe MAGIC telescope has also detected a VHE flare on 24 Sept. 2006 from Cyg X-1 (H.E.S.S. obs. were taken —1 monthearlier). Persistent bi-lobal (~7 arcmin long) 'fossil' jets of 4U1755-33 have been seen in X-rays. This report summarises ourobservations, searching for pointlike VHE emission at the central sources and for extended emission from their jets and/orjet/ISM interaction regions.
机译:许多微奎达表现出Parsec-Scale喷射,其中已知在某些情况下与星际介质(ISM)相互作用。一个名的例子是SS-433系统。在这里,我们总结了H.E.S.在该类别中的三个进一步示例的观察,具有弧形分钟尺度喷射和/或喷射/ ISM交互特征。 CIR X-1喷射Makesthis的小型视角源是潜在的“微柏拉明”。 Cyg X-1喷气机吹出了一个弧形的弓形电击无线电功能,魔法望远镜还从2006年9月24日从Cyg X-1(Hess Obs,拍摄了VHE Flare。 。在X射线中看到持久性双叶(〜7 arcmin long)'Fossil'喷射器4u1755-33。本报告总结了OuroBservations,在中央源的发射点以及延长其喷射器和/ ORJET / ISM互动区域的扩展发射。

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