文章基本信息

标题：Extragalactic Jets
本地全文：下载
作者：G. Ghisellini
期刊名称：PoS - Proceedings of Science
印刷版ISSN：1824-8039
出版年度：2011
卷号：2011
期号：Extremesky2011
出版社：SISSA, Scuola Internazionale Superiore di Studi Avanzati
摘要：The Fermi, Swift and INTEGRAL satellites, together with ground based (especially Cherenkov) telescopes made possible a great progress in our understanding of relativistic jets. We can now start to attack the difficult questions of jet formation, collimation and content. We can also use them as probes to quantify the amount of IR and optical background radiation, and the amount of the cosmic magnetic field. Since they are the most powerful steady sources of the Universe, we can study them also at large redshifts, and this is a very fruitful field of research. To this aim, I will emphasize the importance of high energy X–rays, where very powerful blazars are predicted to emit most of their electromagnetic power. For them, the contribution of the underlying accretion disk is not overwhelmed by the non-thermal jet radiation, allowing to estimate the black hole mass and the accretion rate. In turn, this highlights the connection between the disk and the jet. Since the highest power blazars could have their emission peak in the ∼MeV band, hard X–ray instruments could be more appropriate than the Fermi/LAT to detect them.