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Titlebook: Diffuse Matter in Galaxies; Cargèse 1982 J. Audouze,J. Lequeux,A. Vidal-Madjar Book 1983 D. Reidel Publishing Company, Dordrecht, Holland 1

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書(shū)目名稱Diffuse Matter in Galaxies
副標(biāo)題Cargèse 1982
編輯J. Audouze,J. Lequeux,A. Vidal-Madjar
視頻videohttp://file.papertrans.cn/279/278998/278998.mp4
叢書(shū)名稱Nato Science Series C:
圖書(shū)封面Titlebook: Diffuse Matter in Galaxies; Cargèse 1982 J. Audouze,J. Lequeux,A. Vidal-Madjar Book 1983 D. Reidel Publishing Company, Dordrecht, Holland 1
描述The study of the interstellar medium is certainly one of the most recently developed astrophysical topics. Indeed, to understand the physical status of this medium, one should observe it at every wavelength, especially in radio and in the ranges which are only accessible from space such as Infra Red, X and gammas. Thanks to many new observations we now know that interstellar gas is quite inhomogeneous, since it is made from relatively cold and dense phases (interstellar clouds), surrounded by a relatively hot and tenuous medium. The summer school which took place from September 1 to 16 at the Institut d‘Etudes Scientifiques of Cargese, and from which this book originates, was devoted to the analysis of this second diffuse, hot and tenuous component. The eleven sets of lectures which were presented at this school constitute the chapters of this book. They review different aspects (observations, determination of the physical properties and evolution) of this diffuse medium. In the first chapter, J. Lequeux (Marseille Observatory) introduces the study of the diffuse interstellar medium which plays a major role in galactic evolution. His contribution provides some historical references
出版日期Book 1983
關(guān)鍵詞Galaxy; interstellar matter; observatory; spectroscopy; stellar
版次1
doihttps://doi.org/10.1007/978-94-009-7183-7
isbn_softcover978-94-009-7185-1
isbn_ebook978-94-009-7183-7Series ISSN 1389-2185
issn_series 1389-2185
copyrightD. Reidel Publishing Company, Dordrecht, Holland 1983
The information of publication is updating

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Dynamics and Energetics of the Interstellar Medium,locks are then applied to model idealized versions of localized dynamical situations in the diffuse interstellar medium. Some observational constraints on global models of the interstellar medium are briefly discussed.
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Recycling and trade of waste paper in Indiat review the basic knowledge of the stellar winds (Section II). The theory of the interaction between the wind and the ISM and the structure of a typical interstellar bubble (IB) from a single star is discussed in Section III. A typical example of an observed bubble, the Cygnus Superbubble, is discussed in Section IV.
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https://doi.org/10.1007/978-3-642-95768-0e briefly described in Section III. The evolution of the remnants is discussed in Section IV. In Section V I discuss the effect of supernovae when they occur in stellar clusters. In Section VI the overall effect of stellar winds and supernovae on the interstellar medium is described.
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1389-2185 ry) introduces the study of the diffuse interstellar medium which plays a major role in galactic evolution. His contribution provides some historical references978-94-009-7185-1978-94-009-7183-7Series ISSN 1389-2185
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Book 1983tions, determination of the physical properties and evolution) of this diffuse medium. In the first chapter, J. Lequeux (Marseille Observatory) introduces the study of the diffuse interstellar medium which plays a major role in galactic evolution. His contribution provides some historical references
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