| 书目名称 | The Formation and Disruption of Black Hole Jets |
| 编辑 | Ioannis Contopoulos,Denise Gabuzda,Nikolaos Kylafi |
| 视频video | |
| 概述 | Presents most recent observational results of jet systems in X-ray binaries and AGNs.Discusses most recent theoretical approaches to understanding the physics in these systems.Provides the first steps |
| 丛书名称 | Astrophysics and Space Science Library |
| 图书封面 |  |
| 描述 | .This book reviews the phenomenology displayed by relativistic jets as well as the most recent theoretical efforts to understand the physical mechanisms at their origin. Relativistic jets have been observed and studied in Active Galactic Nuclei (AGN) for about half a century and are believed to be fueled by accretion onto a supermassive black hole at the center of the host galaxy. Since the first discovery of relativistic jets associated with so-called "micro-quasars" much more recently, it has seemed clear that much of the physics governing the relativistic outflows in stellar X-ray binaries harboring black holes and in AGN must be common, but acting on very different spatial and temporal scales. With new observational and theoretical results piling up every day, this book attempts to synthesize a consistent, unified physical picture of the formation and disruption of jets in accreting black-hole systems..The chapters in this book offer overviews accessible not only to specialists but also to graduate students and astrophysicists working in other areas. Covered topics comprise.Relativistic jets in stellar systems.Launching of AGN jets.Parsec-scale AGN jets.Kiloparsec-scale AGN jet |
| 出版日期 | Book 2015 |
| 关键词 | AGN Jets; Accretion Disks; Active Galactic Nuclei; Black Hole Magnetospheres; Cosmic Battery; Formation o |
| 版次 | 1 |
| doi | https://doi.org/10.1007/978-3-319-10356-3 |
| isbn_softcover | 978-3-319-34995-4 |
| isbn_ebook | 978-3-319-10356-3Series ISSN 0067-0057 Series E-ISSN 2214-7985 |
| issn_series | 0067-0057 |
| copyright | Springer International Publishing Switzerland 2015 |
发表于 2025-3-21 17:37:32
