Late Stages of Stellar Evolution: Computational Methods in Astrophysical Hydrodynamics Proceedings of the Astrophysics School II, Organized by the Eu (Springer Proceedings in Physics) by Camiel W. H. De Loore

Cover of: Late Stages of Stellar Evolution: Computational Methods in Astrophysical Hydrodynamics | Camiel W. H. De Loore

Published by Springer .

Written in English

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Subjects:

  • Astronomy - Star Guides,
  • Science

Book details

The Physical Object
FormatHardcover
Number of Pages390
ID Numbers
Open LibraryOL9060580M
ISBN 103540536205
ISBN 109783540536208

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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 Buy Late Stages of Stellar Evolution: Computational Methods in Astrophysical Hydrodynamics: Proceedings of the Astrophysical School II Organized by the (Lecture Notes in Physics, ) on wrcch2016.com FREE SHIPPING on qualified orders.

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De Loore, European Astrophysics Doctoral Network. Book Review: Late stages of stellar evolution, computational methods in astrophysical hydrodynamics / Springer, The ADS is operated by the Smithsonian Astrophysical Observatory under NASA Cooperative Agreement NNX16AC86A.

Resources About ADS ADS Help. Get this from a library. Late stages of stellar evolution: computational methods in astrophysical hydrodynamics: proceedings of the Astrophysics School Late Stages of Stellar Evolution: Computational Methods in Astrophysical Hydrodynamics book, organized by the European Astrophysics Doctoral Network at Ponte de Lima, Portugal, September [Camiel W H de Loore; European Astrophysics Doctoral Network.;].

Title: Book Review: Late stages of stellar evolution, computational methods in astrophysical hydrodynamics / Springer, Book Authors: de Loore, B.

Title: Book-Review - Late Stages of Stellar Evolution Computational Methods in Astrophysical Hydrodynamics - Lecture Notes in Physics Authors.

Jun 21,  · Cite this paper as: Benz W. () An introduction to computational methods in hydrodynamics. In: de Loore C.B. (eds) Late Stages of Stellar Evolution Computational Methods in Astrophysical wrcch2016.com by: 5.

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In this report, the Astro Science Frontiers Panel on Stars and Stellar Evolution sketches the most fertile opportunities for the coming decade in the field of stars and stellar evolution.

Stellar evolution codes, in contrast, use implicit integration schemes to follow the changes in internal structure of a star on thermal and nuclear time scales.

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A predictive computational capability for the effects of turbulent mass, momentum, energy and species transport, as well as material mixing, on the thermonuclear fusion process in ICF entails the development of turbulent transport and mixing or subgrid-scale models based on statistically-averaged or filtered evolution equations, respectively.The book provides a comprehensive treatment of the physics of the stellar interior and the underlying fundamental processes and parameters.

The models developed to explain the stability, dynamics and evolution of the stars are presented and great care is taken to detail the various stages in a star’s life.Plewa, Tomasz A (PI).

(Jul ). The Role of Plasma Self-Magnetization During Late Stages of Stellar Evolution and Stellar Explosions. Submitted to National Aeronautics & Space Administration. Postdoctoral Supervision Handy, T.

(May –Apr ). Flaig, M. (Apr –Mar ). Additional Research or Original Creative Work Not Reported.

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