| 書目名稱 | Magnetic Fields and Star Formation | | 副標(biāo)題 | Theory Versus Observ | | 編輯 | A. I. Gómez Castro,M. Heyer,R. E. Pudritz | | 視頻video | http://file.papertrans.cn/622/621226/621226.mp4 | | 圖書封面 |  | | 描述 | .Magnetic Fields play a key role in the physics of star formation on all scales: from the formation of the large complexes of molecular clouds to the formation of solar-like planetary systems. The plasma physics involved is non-linear and very complex, which requires the development of large numerical codes. An additional difficulty is that the detection and study of magnetic fields is not easy from an observational point of view, and therefore theoretical models cannot easily be constrained. ..In the week from April 21st to 25th in 2003, a meeting was held on the Campus of the Universidad Complutense de Madrid (Spain) to join theoretical and observational efforts to address these issues. The objective was to define a set of relevant problems for the physics of star formation that can be properly addressed with the current or near-future instruments. ..This book summarizes the results of this intensive week of work. The book is written in a comprehensive manner and reviews our current knowledge of the subject. It also represents an updated account of the ideas and thoughts of the scientists working in the field of Star Formation. The contributions are presented in six chapters whic | | 出版日期 | Book 2004 | | 關(guān)鍵詞 | Accretion; instruments; relativistic jet; star; stellar | | 版次 | 1 | | doi | https://doi.org/10.1007/978-94-017-0491-5 | | isbn_softcover | 978-90-481-6602-2 | | isbn_ebook | 978-94-017-0491-5 | | copyright | Springer Science+Business Media Dordrecht 2004 |
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