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Titlebook: High-Velocity Clouds; Hugo Woerden,Bart P. Wakker,Klaas S. Boer Book 2005 Springer Science+Business Media B.V. 2005 Missing Link.Pet.devel

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發(fā)表于 2025-3-21 18:52:06 | 只看該作者 |倒序?yàn)g覽 |閱讀模式
書目名稱High-Velocity Clouds
編輯Hugo Woerden,Bart P. Wakker,Klaas S. Boer
視頻videohttp://file.papertrans.cn/427/426809/426809.mp4
叢書名稱Astrophysics and Space Science Library
圖書封面Titlebook: High-Velocity Clouds;  Hugo Woerden,Bart P. Wakker,Klaas S. Boer Book 2005 Springer Science+Business Media B.V. 2005 Missing Link.Pet.devel
描述On the occasion of the retirement of Ulrich Schwarz, a symposium was held in Groningen in May of 1996, celebrating his contributions to the study of the int- stellar medium, including his work on the high-velocity clouds. The coming together of many specialists in the latter ?eld prompted the idea of compiling a book c- taining their contributions, and summarizing the status of our understanding of the high-velocity cloud phenomenon. This seemed especially worthwhile at the time, since many exciting developments were taking place. After the discovery of some H i clouds with high velocities, about 40 years ago, the subject had been dominated by 21-cm observations of H i emission. Starting in the mid-1980s much progress was being made because of the availability of new instruments, such as large ground-based optical telescopes and UV observatories in space. The connections between the work on high-velocity clouds and other studies of the properties of the (hot) interstellar medium also became clearer.
出版日期Book 2005
關(guān)鍵詞Missing Link; Pet; development; distribution; environment; galaxy; hydrogen; iron; kinematics; milky way; mole
版次1
doihttps://doi.org/10.1007/1-4020-2579-3
isbn_softcover978-90-481-6685-5
isbn_ebook978-1-4020-2579-2Series ISSN 0067-0057 Series E-ISSN 2214-7985
issn_series 0067-0057
copyrightSpringer Science+Business Media B.V. 2005
The information of publication is updating

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沙發(fā)
發(fā)表于 2025-3-21 21:26:30 | 只看該作者
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發(fā)表于 2025-3-22 03:33:27 | 只看該作者
HVCS Related to the Magellanic System,sed on either tidal or ram-pressure forces, with more sophisticated models using a combination of these forces. The Magellanic complexes account for the majority of the HVCs at positive velocities and serve as useful “standard candles” for the HVC population as a whole. They are also important current tracers of the galaxy formation process.
地板
發(fā)表于 2025-3-22 04:55:26 | 只看該作者
The Hot Halo,ites. This chapter reviews the essentials of both absorption and emission by hot halo gas as well as theories for origin and properties of the hot phase. The large body of results on the hot Galactic Halo obtained with FUSE using extragalactic sight lines is summarized at the end.
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發(fā)表于 2025-3-22 10:16:51 | 只看該作者
High-Velocity Clouds: The Missing Link?, for the Local Group origin of the HVCs and its implications for the formation and the evolution of our Galaxy. We describe recent observations that confirm many earlier predictions and discuss future tests of the model.
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發(fā)表于 2025-3-22 13:43:10 | 只看該作者
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發(fā)表于 2025-3-23 00:11:05 | 只看該作者
The Large- and Small-scale Structure of HVCs,the concept of fractality. In general, these methods show a tendency for HVCs to have more pronounced small-scale structure than lower-velocity gas. However, the differences are not so pronounced that it is possible to easily distinguish between high- and low-velocity gas.
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