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Titlebook: Magnetic Fields and Star Formation; Theory Versus Observ A. I. Gómez Castro,M. Heyer,R. E. Pudritz Book 2004 Springer Science+Business Medi

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发表于 2025-3-21 18:29:18 | 显示全部楼层 |阅读模式
书目名称Magnetic Fields and Star Formation
副标题Theory Versus Observ
编辑A. I. Gómez Castro,M. Heyer,R. E. Pudritz
视频video
图书封面Titlebook: Magnetic Fields and Star Formation; Theory Versus Observ A. I. Gómez Castro,M. Heyer,R. E. Pudritz Book 2004 Springer Science+Business Medi
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
关键词Accretion; instruments; relativistic jet; star; stellar
版次1
doihttps://doi.org/10.1007/978-94-017-0491-5
isbn_softcover978-90-481-6602-2
isbn_ebook978-94-017-0491-5
copyrightSpringer Science+Business Media Dordrecht 2004
The information of publication is updating

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Turbulence in the Star-Forming Interstellar Medium: Steps Toward Constraining Theories with Observat a rapid pace, aided in part by numerical simulations. These increased capabilities on both fronts open new opportunities for strengthening the links between observation and theory, and for meaningful comparisons between the two.
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The Tiny-Scale Atomic Structure: Gas Cloudlets or Scintillation Phenomenon ?ns of B0823+26 and B1133+16 are similar on scales of 10–20, 350 and 500 AU. The large number of non detections of the tiny scale atomic structure suggests that the AU-sized structure is not ubiquitous in the interstellar medium.
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Magnetic Flux Transport in the ISM through Turbulent Ambipolar Diffusionether turbulence can enhance the ambipolar diffusion rate sufficiently to explain the observed weak correlations. The numerical method is based on a gas-kinetic scheme with very low numerical diffusivity, thus allowing us to separate numerical and physical diffusion effects.
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