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Titlebook: Stellar Interiors; Physical Principles, Carl J. Hansen,Steven D. Kawaler,Virginia Trimble Textbook 2004Latest edition Springer Science+Busi

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发表于 2025-3-21 19:03:32 | 显示全部楼层 |阅读模式
书目名称Stellar Interiors
副标题Physical Principles,
编辑Carl J. Hansen,Steven D. Kawaler,Virginia Trimble
视频video
概述Includes supplementary material:
丛书名称Astronomy and Astrophysics Library
图书封面Titlebook: Stellar Interiors; Physical Principles, Carl J. Hansen,Steven D. Kawaler,Virginia Trimble Textbook 2004Latest edition Springer Science+Busi
描述The?rsteditionofthistextappearedin1994.Shortlyafterthethirdprinting, our editor suggested that we attempt a second edition because new devel- mentsinstellarstructureandevolutionhadmadeouroriginalworkoutdated. We (the original authors, CJH and SDK) reluctantly agreed but with res- vations due to the e?ort involved. Our initial reluctance disappeared when we were able to convince (cajole, twist the arm of, etc.) our new coauth- colleague Virginia Trimble to join us. (Welcome Virginia!) We (i.e., all three of us) hope that you agree that the present edition is a great improvement compared to the 1994 e?ort. Our objectives in this edition are the same ones we set forth in 1994: Whatyouwill?ndisatextdesignedforourtargetaudience:thety- cal senior undergraduate or beginning graduate student in astronomy or astrophysics who wishes an overview of stellar structure and e- lution with just enough detail to understand the general picture. She or he can go on from there to more specialized texts or directly to the research literature depending on talent and interests. To this end, this text presents the basic physical principles without chasing all the (interesting!) details. For those of you f
出版日期Textbook 2004Latest edition
关键词Evolution; Stellar Structure; asteroseismology; helioseismology; stellar
版次2
doihttps://doi.org/10.1007/978-1-4419-9110-2
isbn_softcover978-1-4612-6497-2
isbn_ebook978-1-4419-9110-2Series ISSN 0941-7834 Series E-ISSN 2196-9698
issn_series 0941-7834
copyrightSpringer Science+Business Media New York 2004
The information of publication is updating

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Preliminaries,lly gives rise to the radiation we see streaming off the surface. The vast majority of stars spend most of their active lives in such an equilibrium state, converting hydrogen into helium, and it is only this gradual transmutation of elements by the fusion process that eventually causes their struct
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Asteroseismology,radius, and color variations to probe stellar interiors in much the same spirit as in terrestrial seismology. This is not a new subject but it has blossomed in recent years. A review of the list of variables we gave in Chapter 2 makes it clear that the subject spans all phases of stellar evolution.
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Structure and Evolution of White Dwarfs, as the endpoint of evolution for most stars. The variable white dwarfs, discussed in the final section, will be shown to play an important role in this program. There is no one text that deals solely with these objects but, for further reading, we suggest (1980), (1983), (1984), (1990), (1990), (1990), (1991), (1992), (2001), (2002), and (2003).
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0941-7834 second edition because new devel- mentsinstellarstructureandevolutionhadmadeouroriginalworkoutdated. We (the original authors, CJH and SDK) reluctantly agreed but with res- vations due to the e?ort involved. Our initial reluctance disappeared when we were able to convince (cajole, twist the arm of,
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