Late stages of stellar evolution : computational methods in astrophysical hydrodynamics : proceedings of the Astrophysics School II, organized by the European Astrophysics Doctoral Network at Ponte de Lima, Portugal, 11-23 September 1989 / C.B. de Loore, ed.
Contributor(s): Loore, Camiel W. H. de | European Astrophysics Doctoral NetworkMaterial type: TextSeries: Lecture notes in physics: 373.Publisher: Berlin ; New York : Springer-Verlag, ©1991Description: 1 online resource (viii, 390 pages) : illustrationsContent type: text Media type: computer Carrier type: online resourceISBN: 9783540469216; 3540469214Subject(s): Stars -- Evolution -- Congresses | Hydrodynamics -- Congresses | Astrophysics -- Congresses | Astrophysics | Hydrodynamics | Stars -- Evolution | Estrelas (agrupamento e associacoes) | Astrofisica | Étoiles -- Évolution -- Congrès | Astrophysique -- CongrèsGenre/Form: Electronic books. | Conference papers and proceedings. Additional physical formats: Print version:Astrophysics School (2nd : 1989 : Ponte do Lima, Portugal).: Late stages of stellar evolution.DDC classification: 523.8 LOC classification: QB806 | .A88 1989Online resources: Click here to access online
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Includes bibliographical references.
Stellar structure and stellar evolution / Bert C. de Loore -- Supernovae : observations, theory, models and nucleosynthesis / Ewald Muller -- Circumstellar envelopes of late type stars / Alain Omont -- Evolution of close binary systems : application to X-ray binaries / Gertjan J. Savonije -- An introduction to computational methods in hydrodynamics / Willy Benz -- Basic hydrodynamics / Jean Heyvaerts -- Convection and turbulence in stars / Jean-Paul Zahn.
This collection of 7 lectures is intended to be a textbook for graduate students who want to learn about modern developments in astronomy and astrophysics. The first part surveys various aspects of the late stages of stellar evolution, including observation and theory. B.C. de Loore's long article on stellar structure is followed by reviews on supernovae, on circumstellar envelopes, and on the evolution of binaries. The second part deals with the important problem of modeling stellar evolution based on the computational hydrodynamics.
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