| 書目名稱 | Protostellar Jets in Context |
| 編輯 | Kanaris Tsinganos,Tom Ray,Matthias Stute |
| 視頻video | http://file.papertrans.cn/763/762008/762008.mp4 |
| 概述 | Latest on astrophysical jet research.Exceptional collection of contributions by all leaders in the field.Includes supplementary material: |
| 叢書名稱 | Astrophysics and Space Science Proceedings |
| 圖書封面 |  |
| 描述 | It is over a quarter of a century since the discovery of out?ows from young stars. The intervening years have led to remarkable advances in our understanding of this phenomenon. Much of the progress can be attributed to advances in facilities and technologies, including not only larger telescopes but also improved instrument and detector performance. In addition protostellar out?ows have now been imaged from the ground and space at high spatial resolution, e. g. with HST, and at a wide - riety of wavelengths from X-rays to radio waves, revealing more and more about their physics. This veritable revolution in observation has been accompanied by an exponential growth in our ability to numerically simulate the launching and pro- gation of jets. Codes continue to improve: they now incorporate more physics and are increasingly ef?cient through, for example, techniques such as adaptive mesh re?nement and the use of parallel processing in cluster environments. Simulating the launching and propagation of a jet all the way from the vicinity of the star up to 4 several thousand AU (a size range of10 ) is now much closer. In more recent times, developments in observation, theory and numerical |
| 出版日期 | Conference proceedings 2009 |
| 關(guān)鍵詞 | Accretion; Accretion - Ejection; Accretion Disks; Magneto-rotational instability; Magnetohydrodynamic je |
| 版次 | 1 |
| doi | https://doi.org/10.1007/978-3-642-00576-3 |
| isbn_softcover | 978-3-642-26117-6 |
| isbn_ebook | 978-3-642-00576-3Series ISSN 1570-6591 Series E-ISSN 1570-6605 |
| issn_series | 1570-6591 |
| copyright | Springer-Verlag Berlin Heidelberg 2009 |
|Archiver|手機(jī)版|小黑屋|
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