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

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 arti...

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Bibliographic Details
Other Authors: Loore, C.B. de (Editor)
Format: eBook
Language:English
Published: Berlin, Heidelberg Springer Berlin Heidelberg 1991, 1991
Edition:1st ed. 1991
Series:Lecture Notes in Physics
Subjects:
Online Access:
Collection: Springer Book Archives -2004 - Collection details see MPG.ReNa
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245 0 0 |a Late Stages of Stellar Evolution Computational Methods in Astrophysical Hydrodynamics  |h Elektronische Ressource  |b Proceedings of the Astrophysics School II Organized by the European Astrophysics Doctoral Network at Ponte de Lima Portugal, 11–23 September 1989  |c edited by C.B. de Loore 
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505 0 |a Stellar structure and stellar evolution -- Supernovae: Observations, theory, models and nucleosynthesis -- Circumstellar envelopes of late type stars -- Evolution of close binary systems: Application to X-ray binaries -- An introduction to computational methods in hydrodynamics -- Basic hydrodynamics -- Convection and turbulence in stars 
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653 |a Mathematical physics 
653 |a Astronomy, Observations and Techniques 
653 |a Astrophysics 
653 |a Theoretical, Mathematical and Computational Physics 
653 |a Mathematical Methods in Physics 
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490 0 |a Lecture Notes in Physics 
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520 |a 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