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Titlebook: Galactic and Intergalactic Magnetic Fields; Ulrich Klein,Andrew Fletcher Book 2015 Springer International Publishing Switzerland 2015 Astr

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發(fā)表于 2025-3-21 20:08:02 | 只看該作者 |倒序?yàn)g覽 |閱讀模式
書(shū)目名稱(chēng)Galactic and Intergalactic Magnetic Fields
編輯Ulrich Klein,Andrew Fletcher
視頻videohttp://file.papertrans.cn/381/380340/380340.mp4
概述Conveys the fundamentals of magnetic fields and relativistic plasma in diffuse cosmic media.Addresses theoretical concepts wherever necessary.Discusses the role of magnetic fields in the evolution of
叢書(shū)名稱(chēng)Springer Praxis Books
圖書(shū)封面Titlebook: Galactic and Intergalactic Magnetic Fields;  Ulrich Klein,Andrew Fletcher Book 2015 Springer International Publishing Switzerland 2015 Astr
描述This course-tested textbook conveys the fundamentals of magnetic fields and relativistic plasma in diffuse cosmic media, with a primary focus on phenomena that have been observed at different wavelengths. Theoretical concepts are addressed wherever necessary, with derivations presented in sufficient detail to be generally accessible..In the first few chapters the authors present an introduction to various astrophysical phenomena related to cosmic magnetism, with scales ranging from molecular clouds in star-forming regions and supernova remnants in the Milky Way, to clusters of galaxies. Later chapters address the role of magnetic fields in the evolution of the interstellar medium, galaxies and galaxy clusters..The book is intended for advanced undergraduate and postgraduate students in astronomy and physics and will serve as an entry point for those starting their first research projects in the field.
出版日期Book 2015
關(guān)鍵詞Astrophysical Magnetic Fields Textbook; Continuum Radiation Processes; Cosmological Magnetic Fields; Ga
版次1
doihttps://doi.org/10.1007/978-3-319-08942-3
isbn_softcover978-3-319-34671-7
isbn_ebook978-3-319-08942-3
copyrightSpringer International Publishing Switzerland 2015
The information of publication is updating

書(shū)目名稱(chēng)Galactic and Intergalactic Magnetic Fields影響因子(影響力)




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978-3-319-34671-7Springer International Publishing Switzerland 2015
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Gerald C. Cupchik,R. Walter Heinrichsthat the nonthermal component with its power-law spectrum is synchrotron radiation (free-free emission preponderates in the Galatic plane and in HII regions), and that a magnetic field must be ubiquitously present in the Milky Way.
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Erwan Josse,Pascal Bach,Laurent Dagornential made up by stars and dark matter. In spiral galaxies, the gas has a neutral and an ionised phase. The neutral phase is made up by (in order of decreasing density) the molecular medium, the cold neutral medium (CNM), and the warm neutral medium (WNM). The ionised phase consists of the warm (WIM) and the hot (HIM) ionised medium (Table 5.1).
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The Evidence Regarding ACL Repair,c field. As pointed out in Sect.?5.5, their synchrotron luminosity is closely associated with the star formation in their disks, this giving rise to the well-known radio-FIR correlation established for star-forming galaxies.
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Magnetic Fields in Galaxies,ential made up by stars and dark matter. In spiral galaxies, the gas has a neutral and an ionised phase. The neutral phase is made up by (in order of decreasing density) the molecular medium, the cold neutral medium (CNM), and the warm neutral medium (WNM). The ionised phase consists of the warm (WIM) and the hot (HIM) ionised medium (Table 5.1).
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