| 書目名稱 | Physics of Active Galactic Nuclei at all Scales | | 編輯 | Danielle Alloin,Rachel Johnson,Paulina Lira | | 視頻video | http://file.papertrans.cn/748/747135/747135.mp4 | | 叢書名稱 | Lecture Notes in Physics | | 圖書封面 |  | | 描述 | The study of the physical processes at work in Active Galactic Nuclei (AGN) has kept a large number of astronomers busy since the discovery, in the early sixties, of the ?rst radio galaxies and quasars. After a few decades of debate there is now a clear consensus about the source of energy in AGN, namely gravitational energy released through matter accretion onto a massive black hole. The most commonly accepted ideas regarding AGN are pictured in the so-called AGN uni?ed model, although one should remember that this is still a “working” model. Tremendous progress has been made in unveiling, analyzing, and modeling the di?erent components in AGN: the accretion disk, the jets of relativistic particles, the x-ray absorber close to the central engine,the“torus”thatfunnelstheionizingradiation,thesurroundingclouds of dense material in the broadline region and narrowline region, the cool molecular and dusty material around the torus, as well as jet-induced e?ects on larger scales. Yet, it remains to incorporate all these components and physical processes into a self-consistent AGN model that would take into account, and predict, all the facets of AGN activity. The mere process of matter f | | 出版日期 | Book 2006 | | 關(guān)鍵詞 | AGN; Galaxy; Quasar; X-ray; accretion disks; active galactic nuclei; broad-line region; relativistic jet; st | | 版次 | 1 | | doi | https://doi.org/10.1007/b11550280 | | isbn_softcover | 978-3-642-06833-1 | | isbn_ebook | 978-3-540-34621-0Series ISSN 0075-8450 Series E-ISSN 1616-6361 | | issn_series | 0075-8450 | | copyright | Springer-Verlag Berlin Heidelberg 2006 |
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