Stars and Stellar Evolution

The diverse forms that stars assume in the course of their lives can all be derived from the initial conditions : the mass and the original chemical composition. In this textbook Stars and Stellar Evolution the basic concepts of stellar structure and the main roads of stellar evolution are described...

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Hauptverfasser: de Boer, Klaas (VerfasserIn), Seggewiss, Wilhelm (VerfasserIn)
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Sprache:English
Veröffentlicht: Les Ulis EDP Sciences [2021]
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Datensatz im Suchindex

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spelling de Boer, Klaas Verfasser aut
Stars and Stellar Evolution Wilhelm Seggewiss, Klaas de Boer
Les Ulis EDP Sciences [2021]
© 2008
1 online resource (332 pages)
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Description based on online resource; title from PDF title page (publisher's Web site, viewed 25. Feb 2021)
The diverse forms that stars assume in the course of their lives can all be derived from the initial conditions : the mass and the original chemical composition. In this textbook Stars and Stellar Evolution the basic concepts of stellar structure and the main roads of stellar evolution are described. First, the observable parameters are presented, which are based on the radiation emerging from a stellar atmosphere. Then the basic physics is described, such as the physics of gases, radiation transport, and nuclear processes, followed by essential aspects of modelling the structure of stars. After a chapter on star formation, the various steps in the evolution of stars are presented. This leads us to brown dwarfs, to the way a star changes into the red-giant state and numerous other stages of evolution and ultimately to the stellar ashes such as white dwarfs, supernovae and neutron stars. Stellar winds, stellar rotation and convection all influence the way a star evolves. The evolution of binary stars is included by using several canonical examples in which interactive processes lead to X-ray binaries and supernovae of type Ia. Finally, the consequences of the study of stellar evolution are tied to observed mass and luminosity functions and to the overall evolution of matter in the universe. The authors aim at reaching an understanding of stars and their evolution by both graduate students and astronomers who are not themselves investigating stars. To that end, numerous graphs and sketches, among which the Hertzsprung-Russell diagram is the dominant one, help trace the ways of stellar evolution. Ample references to specialised review articles as well as to relevant research papers are included
In English
Astrophysics
SCIENCE / Physics / Astrophysics bisacsh
Sternentwicklung (DE-588)4057365-5 gnd rswk-swf
Stellarastronomie (DE-588)4193384-9 gnd rswk-swf
Sternentwicklung (DE-588)4057365-5 s
DE-604
Stellarastronomie (DE-588)4193384-9 s
Seggewiss, Wilhelm aut
Erscheint auch als Druck-Ausgabe 9782759803569
https://www.degruyter.com/isbn/9782759803286 Verlag URL des Erstveröffentlichers Volltext
spellingShingle de Boer, Klaas
Seggewiss, Wilhelm
Stars and Stellar Evolution
Astrophysics
SCIENCE / Physics / Astrophysics bisacsh
Sternentwicklung (DE-588)4057365-5 gnd
Stellarastronomie (DE-588)4193384-9 gnd
subject_GND (DE-588)4057365-5
(DE-588)4193384-9
title Stars and Stellar Evolution
title_auth Stars and Stellar Evolution
title_exact_search Stars and Stellar Evolution
title_exact_search_txtP Stars and Stellar Evolution
title_full Stars and Stellar Evolution Wilhelm Seggewiss, Klaas de Boer
title_fullStr Stars and Stellar Evolution Wilhelm Seggewiss, Klaas de Boer
title_full_unstemmed Stars and Stellar Evolution Wilhelm Seggewiss, Klaas de Boer
title_short Stars and Stellar Evolution
title_sort stars and stellar evolution
topic Astrophysics
SCIENCE / Physics / Astrophysics bisacsh
Sternentwicklung (DE-588)4057365-5 gnd
Stellarastronomie (DE-588)4193384-9 gnd
topic_facet Astrophysics
SCIENCE / Physics / Astrophysics
Sternentwicklung
Stellarastronomie
url https://www.degruyter.com/isbn/9782759803286
work_keys_str_mv AT deboerklaas starsandstellarevolution
AT seggewisswilhelm starsandstellarevolution