2007/07/09 by R. M. Sambruna, Sambruna, R. M., D. Donato +7
Engineering · Physics and Astronomy · #Astrophysical Phenomena and Observations #Astrophysics (astro-ph) #Astrophysics and Cosmic Phenomena #FOS: Physical sciences #Particle Accelerators and Free-Electron Lasers #astro-ph
paper · pdf · doi:10.48550/arxiv.0707.1321
5 pages, 2 figures, to be published in the Proceedings of the conference "Extragalactic Jets - Theory and Observation from Radio to Gamma Ray-", May 21-24 2007, Girdwood, Alaska; revised authorship
openalex publication_date 2007/07/09 · arxiv created 2007/07/10 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
The BL Lac S5 2007+777 was observed by us with Chandra, to find the X-ray counterpart to its 18" radio jet, and study its structure. Indeed, a bright X-ray jet was discovered in the 33 ks ACIS-S image of the source. We present its properties and briefly discuss the implications.