Titlebook: Astrophysical Radiation Hydrodynamics; Karl-Heiz A. Winkler,Michael L. Norman Book 1986 D. Reidel Publishing Company, Dordrecht, Holland 1

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https://doi.org/10.1007/978-1-4302-0120-5 while the Lagrangian observer is one at rest in the fluid. We can define an observer at an event in spacetime by giving his 4-velocity at that event. The path through spacetime taken by the observer is called the timeline of that observer. In flat Minkowski spacetime (the spacetime of special relat

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https://doi.org/10.1007/978-94-009-4754-2astronomy; astrophysics; gravitation; relativity; turbulence

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978-94-010-8612-7D. Reidel Publishing Company, Dordrecht, Holland 1986

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Nato Science Series C:http://image.papertrans.cn/b/image/163684.jpg

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1389-2185 ivistic and relativistic hydrodynamics, radia- tive transfer, and radiation-coupled hydrodynamics. The unifying theme of the lectures was the successful application of these methods to challenging problems in astrophysics. The workshop was subdivided into 3 somewhat independent topics, each with the

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