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Titlebook: Giants of Eclipse: The ζ Aurigae Stars and Other Binary Systems; Thomas B. Ake,Elizabeth Griffin Book 2015 Springer International Publishi

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發(fā)表于 2025-3-21 19:59:33 | 只看該作者 |倒序?yàn)g覽 |閱讀模式
書(shū)目名稱(chēng)Giants of Eclipse: The ζ Aurigae Stars and Other Binary Systems
編輯Thomas B. Ake,Elizabeth Griffin
視頻videohttp://file.papertrans.cn/386/385707/385707.mp4
概述Carefully edited volume reviewing a rare class of eclipsing binary stars.Describes historical development of the field as well as modern observational and theoretical results.Provides detailed informa
叢書(shū)名稱(chēng)Astrophysics and Space Science Library
圖書(shū)封面Titlebook: Giants of Eclipse: The ζ Aurigae Stars and Other Binary Systems;  Thomas B. Ake,Elizabeth Griffin Book 2015 Springer International Publishi
描述.The zeta Aurigae stars are the rare but illustrious sub-group of binary stars that undergo the dramatic phenomenon of "chromospheric eclipse". This book provides detailed descriptions of the ten known systems, illustrates them richly with examples of new spectra, and places them in the context of stellar structure and evolution..Comprised of a large cool giant plus a small hot dwarf, these key eclipsing binaries reveal fascinating changes in their spectra very close to total eclipse, when the hot star shines through differing heights of the "chromosphere", or outer atmosphere, of the giant star. The phenomenon provides astrophysics with the means of analyzing the outer atmosphere of a giant star and how that material is shed into space. The physics of these critical events can be explained qualitatively, but it is more challenging to extract hard facts from the observations, and tough to model the chromosphere in any detail..The book offers current thinking on mechanismsfor heating a star‘s chromosphere and on how a star loses mass, and relates this science synergistically to studies of other stars and binaries, and to the increasing relevance of contributions from new techniques
出版日期Book 2015
關(guān)鍵詞Asteroseismology of Giant Stars; Eclipsing Binary Stars; Giant Star Chromosphere; Stellar Eclipses; Wind
版次1
doihttps://doi.org/10.1007/978-3-319-09198-3
isbn_softcover978-3-319-35676-1
isbn_ebook978-3-319-09198-3Series ISSN 0067-0057 Series E-ISSN 2214-7985
issn_series 0067-0057
copyrightSpringer International Publishing Switzerland 2015
The information of publication is updating

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Living reference work 20200th editionon of winds in single cool, evolved stars and in eclipsing binary stars, including physical models that have recently been proposed. It describes the successes that have been achieved so far by invoking acoustic and MHD waves to provide a physical description of plasma heating and wind acceleration, and discusses the challenges that still remain.
板凳
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Katrin M?ltgen-Sicking,Nicole Najemnikellar disks is helping to solve long-standing problems related to carbon stars, and summarizes some of the state-of-the-art techniques that are now being used to image spots and convective cells on supergiants.
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Atmospheric Heating and Wind Acceleration in Cool Evolved Stars,on of winds in single cool, evolved stars and in eclipsing binary stars, including physical models that have recently been proposed. It describes the successes that have been achieved so far by invoking acoustic and MHD waves to provide a physical description of plasma heating and wind acceleration, and discusses the challenges that still remain.
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發(fā)表于 2025-3-22 10:36:07 | 只看該作者
Optical Interferometry of Giants and Supergiants,ellar disks is helping to solve long-standing problems related to carbon stars, and summarizes some of the state-of-the-art techniques that are now being used to image spots and convective cells on supergiants.
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https://doi.org/10.1007/978-3-658-36629-2 the framework of modern observing, data management and computing, outlines the principal features of the chromospheric-eclipse phenomena which single out the .?Aur?binaries for special study, and describes the considerable potential which this remarkable yet very select group of stars offers for increasing our understanding of stellar physics.
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