EDP Sciences 1776402950 20260417 fre

laboutique.edpsciences.fr-000065 03 01 01 000065 03 9782759803569 15 9782759803569 00 BA 02 1 mm 01 1 mm 08 1 gr 10 01 02 Hors Collection - 01 01 Stars and Stellar Evolution 1 A01 01 A108 Klaas de Boer de Boer, Klaas Klaas de Boer Klaas de Boer specialized in optical and UV interstellar studies as well as in the UV output of old stars. After postdoctoral periods in Madison (WI, USA), Tübingen (Germany)and Herstmonceux (UK) he became professor at and Director of the Sternwarte of the University of Bonn. 2 A01 01 A109 Wilhelm Seggewiss Seggewiss, Wilhelm Wilhelm Seggewiss Wilhelm Seggewiss studied mathematics, physic and astronomy at the universities of München and Münster(Germany) where he got his PhD in astronomy. After postdoctoral assistantship at Münster he joined the staff of the observatory of the university of Bonn. After 1979 he became professor at Bonn and chairman of the observatory. Main fields of research are evolution of star clusters and the atmospheres of massive stars. 1 01 eng 00 314 03 24 Izibook:Subject Astrophysique 24 Izibook:SubjectAndCategoryAndTags |Astrophysique| 10 2011 SCI005000 29 3066 01 520 01 06 05 00 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. 03 00 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. 02 00 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 presente... 21 00 06 01 https://laboutique.edpsciences.fr/produit/65/9782759803286/stars-and-stellar-evolution 01 00 03 02 https://laboutique.edpsciences.fr/system/product_pictures/data/009/981/404/original/Star_and_stellar.jpg 17 14 20240913T172202+0200 15 00 04 02 01 E107 04 0356_som.pdf 05 0.12 06 4864ee15f3178929c9b055764bc5613d https://laboutique.edpsciences.fr/extract/544?filename=0356_som.pdf&md5sum=4864ee15f3178929c9b055764bc5613d&size=123233&title=Sommaire+de+l%27ouvrage 17 14 20140905T164600+0200 16 00 04 01 https://laboutique.edpsciences.fr/extract/544/preview 01 P1 EDP Sciences 01 01 P1 EDP Sciences 17 avenue du Hoggar - PA de Courtaboeuf - 91944 Les Ulis cedex A http://publications.edpsciences.org/ 04 01 00 20081001 19 00 20081001 2026 06 3052868830012 01 WORLD 27 03 9782759803286 15 9782759803286 WORLD 08 EDP Sciences 04 01 00 20081001 03 01 D1 EDP Sciences 21 04 05 01 02 1 00 33.00 01 5.50 1.72 EUR 04 06 01 02 1 00 82.00 01 5.50 1.72 EUR 01 laboutique.edpsciences.fr-R000195 03 01 01 R000195 00 ED E107 02 01 01 Stars and Stellar Evolution 01 eng 08 333 03 22 9485354 17 16 00 06 01 https://laboutique.edpsciences.fr/flip_book/show/179 01 P1 EDP Sciences 01 01 P1 EDP Sciences 17 avenue du Hoggar - PA de Courtaboeuf - 91944 Les Ulis cedex A http://publications.edpsciences.org/ 02 01 000883 03 9782759803286 15 9782759803286 03 01 D1 EDP Sciences 45 03 laboutique.edpsciences.fr-000883 03 01 01 000883 03 9782759803286 15 9782759803286 10 EA E107 10 02 01 R000195 ED E107 1 10 01 02 Hors Collection - 01 01 Stars and Stellar Evolution 1 A01 01 A108 Klaas de Boer de Boer, Klaas Klaas de Boer Klaas de Boer specialized in optical and UV interstellar studies as well as in the UV output of old stars. After postdoctoral periods in Madison (WI, USA), Tübingen (Germany)and Herstmonceux (UK) he became professor at and Director of the Sternwarte of the University of Bonn. 2 A01 01 A109 Wilhelm Seggewiss Seggewiss, Wilhelm Wilhelm Seggewiss Wilhelm Seggewiss studied mathematics, physic and astronomy at the universities of München and Münster(Germany) where he got his PhD in astronomy. After postdoctoral assistantship at Münster he joined the staff of the observatory of the university of Bonn. After 1979 he became professor at Bonn and chairman of the observatory. Main fields of research are evolution of star clusters and the atmospheres of massive stars. 1 01 eng 08 332 03 24 Izibook:Subject Astrophysique 24 Izibook:SubjectAndCategoryAndTags |Astrophysique| 10 2011 SCI005000 29 3066 01 520 01 06 05 00 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. 03 00 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. 02 00 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 presente... 21 00 06 01 https://laboutique.edpsciences.fr/produit/65/9782759803286/stars-and-stellar-evolution 01 00 03 02 https://laboutique.edpsciences.fr/system/product_pictures/data/009/981/404/original/Star_and_stellar.jpg 17 14 20240913T172202+0200 16 00 04 01 https://laboutique.edpsciences.fr/extract/544/preview 01 P1 EDP Sciences 01 01 P1 EDP Sciences 17 avenue du Hoggar - PA de Courtaboeuf - 91944 Les Ulis cedex A http://publications.edpsciences.org/ 04 01 00 20081001 19 00 20081001 2026 06 3052868830012 01 WORLD 13 03 9782759803569 15 9782759803569 WORLD 08 EDP Sciences 04 01 00 20081001 03 01 D1 EDP Sciences 20 04 05 01 02 1 00 22.99 01 5.50 1.20 EUR 04 06 01 02 1 00 78.99 01 5.50 1.20 EUR 01 04 06 01 02 1 00 87.99 01 5.50 4.59 USD 01