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Asymptotic Giant Branch Stars (Astronomy and Astrophysics Library) 🔍
Harm J. Habing, Hans Olofsson (auth.), Harm J. Habing, Hans Olofsson (eds.) Springer-Verlag New York, Astronomy and Astrophysics Library, Astronomy and Astrophysics Library, 1, 2004
英语 [en] · PDF · 18.9MB · 2004 · 📘 非小说类图书 · 🚀/lgli/lgrs/nexusstc/scihub/zlib · Save
描述
This book deals with stars during a short episode before they undergo a ma jor, and fatal, transition. Soon the star will stop releasing nudear energy, it will become a planetary nebula for abrief but poetic moment, and then it will turn into a white dwarf and slowly fade out of sight. Just before this dramatic change begins the star has reached the highest luminosity and the largest diameter in its existence, and while it is a star detectable in galaxies beyond the Local Group, its structure contains already the inconspicuous white dwarf it will become. It is called an "asymptotic giant branch star" or "AGB star". Over the last 30 odd years AGB stars have become a topic of their own although individual members of this dass had already been studied for cen turies without realizing what they were. In the early evolution, so called "E-AGB"-phase, the stars are a bit bluer than, but otherwise very similar to, what are now called red giant branch stars (RGB stars). It is only in the sec ond half of their anyhow brief existence that AGB stars differ fundamentally from RGB stars.
Erscheinungsdatum: 12.12.2011
备用文件名
lgrsnf/A:\Springer\bok%3A978-1-4757-3876-6.pdf
备用文件名
nexusstc/Asymptotic Giant Branch Stars/612b6f230bf4ce2e932d2baf17ae072f.pdf
备用文件名
scihub/10.1007/978-1-4757-3876-6.pdf
备用文件名
zlib/Astronomy/Harm J. Habing, Hans Olofsson (auth.), Harm J. Habing, Hans Olofsson (eds.)/Asymptotic Giant Branch Stars_2250474.pdf
备用出版商
Springer New York : Imprint: Springer
备用出版商
Springer Nature
备用出版商
Springer US
备用版本
Softcover reprint of the original 1st ed. 2004, 2011-03-06
备用版本
Astronomy and astrophysics library, New York, NY, 2004
备用版本
Astronomy and astrophysics library, New York, 2011
备用版本
United States, United States of America
备用版本
Springer Nature, New York, NY, 2013
备用版本
1, 20130417
元数据中的注释
lg1081510
元数据中的注释
{"container_title":"Astronomy and Astrophysics Library","edition":"1","isbns":["1441918434","1475738765","9781441918437","9781475738766"],"issns":["0941-7834"],"last_page":562,"publisher":"Springer New York","series":"Astronomy and Astrophysics Library"}
备用描述
This book deals with the underlying astrophysical mechanisms of the objects known as asymptotic giant branch stars -- the structures that occur during the dramatic period prior to a star's death. Over the past three decades, asymptotic giant branch stars have become a topic of their own, and the contributions to this volume all focus on these entities themselves, rather than their connections to other fields of astronomy. Among the many topics covered are new methods of high- quality infrared observation and the more detailed and realistic simulations made possible by increasingly fast computers. This collection should be useful to graduate students who work in the field, teachers who want to address the subject in their courses, and to astronomers from various backgrounds who are interested in the astrophysics of AGB stars.
备用描述
Front Matter....Pages I-IX
AGB Stars: History, Structure, and Characteristics....Pages 1-21
Evolution, Nucleosynthesis, and Pulsation of AGB Stars....Pages 23-104
Synthetic AGB Evolution....Pages 105-148
Atmospheres of AGB Stars....Pages 149-245
Molecule and Dust Grain Formation....Pages 247-289
Dynamics and Instabilities in Dusty Winds....Pages 291-323
Circumstellar Envelopes....Pages 325-410
AGB Stars as Tracers of Stellar Populations....Pages 411-460
AGB Stars in Binaries and Their Progeny....Pages 461-518
Post-AGB Stars....Pages 519-553
Back Matter....Pages 555-562
备用描述
The underlying astrophysical mechanisms of the objects known as asymptotic giant branch stars - the structures that occur during the dramatic period prior to a star's death - is the main theme of this text.
开源日期
2013-12-12
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