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Titlebook: Kinematics and Dynamics of Diffuse Astrophysical Media; J. E. Dyson,E. B. Carling Book 1994 Springer Science+Business Media Dordrecht 1994

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发表于 2025-3-21 16:21:50 | 显示全部楼层 |阅读模式
书目名称Kinematics and Dynamics of Diffuse Astrophysical Media
编辑J. E. Dyson,E. B. Carling
视频videohttp://file.papertrans.cn/544/543024/543024.mp4
图书封面Titlebook: Kinematics and Dynamics of Diffuse Astrophysical Media;  J. E. Dyson,E. B. Carling Book 1994 Springer Science+Business Media Dordrecht 1994
描述The area of diffuse astrophysical media is enormous and ranges over circum­ stellar to extragalactic scales. The physical conditions can vary from cool dusty gases to collections of relativistic particles. Flows in such media are set up by en­ ergy and momentum injection from winds, jets and explosions. The study of these phenomena involves physics, chemistry and, inevitably, hydrodynamics. One of the most important aspects of this study is the ever increasing overlap between theory and observation. Indeed, it can be argued that the only way to really understand these complex flows which can never be duplicated under terrestrial conditions, is to encourage this overlap, and this was one major aim of this Conference. Because of the long theoretical and observational association of the Manchester Group with this general area, Manchester seemed an appropriate venue for this Con­ ference. But in fact this long association and the actual year of the Conference are connected. In 1951 Franz Kahn joined the Astronomy Department at Manchester University and immediately the study of diffuse media, particularly the hydrody­ namic aspects, commenced and has flourished ever since. Franz became
出版日期Book 1994
关键词LOPES; Population; Variation; active galactic nuclei; cosmic ray; galaxy; gravitation; magnetosphere; nebula
版次1
doihttps://doi.org/10.1007/978-94-011-0926-0
isbn_softcover978-94-010-4399-1
isbn_ebook978-94-011-0926-0
copyrightSpringer Science+Business Media Dordrecht 1994
The information of publication is updating

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Parametric determination of the inclination of Keplerian circumstellar discs from spectropolarimetrcircumstellar disc are presented. It is shown that analysis of the scattered line profiles at different wavelengths which, due to Doppler redistribution, sample different disc regions allows the disc inclination to be determined.
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Jets,s. Recent measurements of the proper motions of HH objects show that even those near the source are moving at about the same speed as the jet fluid. This means that they cannot be due to steady shocks in the jet and the only obvious explanation is that the source is varying.
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Cosmical Gas Dynamics, Why Was It So Difficult?,When the invitation for this meeting reached me, I did not hesitate. Of course, I wished to be present when it was Franz Kahn’s turn for the formal move to say goodbye. Like many of us, he will probably sneak in again through the back door and continue working.
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Complex Structure Associated with the Wolf-Rayet Star WR147,The Wolf-Rayet star WR147 is known to be bright at X-ray and radio wavelengths (van der Hucht ., 1981, Caillaut ., 1985, Abbot ., 1986).
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The Importance of Continuum Radiation for the Stellar Wind Hydrodynamics of Hot Stars,The contribution of bound-free and free-free processes to the outward acceleration of ζPup is studied and is found to be negligible.
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