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Astrophysical Fluid Dynamics and Applications to Stellar Modeling
2018The modeling of astrophysical objects poses a challenging multiscale multiphysics problem. Because of their large spatial extent, the description of physical processes dominating the formation, structure, and evolution of such objects is typically based on effective theories such as fluid dynamics or thermodynamics.
F. Röpke
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Principles of Astrophysical Fluid Dynamics
, 2007 Fluid dynamical forces drive most of the fundamental processes in the Universe and so play a crucial role in our understanding of astrophysics. This comprehensive textbook, first published in 2007, introduces the necessary fluid dynamics to understand a wide range of astronomical phenomena, from stellar structures to supernovae blast waves, to ...
Cathie Clarke, Bob Carswell
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Fundamentals of Astrophysical Fluid Dynamics
Astronomy and Astrophysics Library, 2020Shoji Kato, Jun Fukue
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ZAMM - Journal of Applied Mathematics and Mechanics / Zeitschrift für Angewandte Mathematik und Mechanik, 2023
Rotational buoyancy assumes a substantial role in a multitude of natural and engineering systems, with particular emphasis on astrophysical and geophysical scenarios.
Sanatan Das +4 more
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Rotational buoyancy assumes a substantial role in a multitude of natural and engineering systems, with particular emphasis on astrophysical and geophysical scenarios.
Sanatan Das +4 more
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Computational Astrophysical Fluid Dynamics
Astrophysics and Space Science, 2000zbMATH Open Web Interface contents unavailable due to conflicting licenses.
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Numerical Fluid Dynamics in Astrophysics
2009The matter of astrophysical objects (e. g., a star or a galaxy) can often be approximated as a gas or fluid, i. e., the equations of fluid dynamics are adequate to describe the astrophysical phenomena. Hereafter, for simplification, the word fluid will be used as a synonym for both fluid and gas.
Hillebrandt, W. +2 more
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Topics in Astrophysical Fluid Dynamics
2006This brief description of some fluid dynamical problems of astrophysical interest focuses on two effects that are characteristic of the subject: self-gravity and radiative forces. Self-gravity is important in determining the basic structures of cosmic bodies as well as producing some intriguing instabilities. Radiation, by which we observe these bodies,
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On dynamics of fluids in astrophysics
Journal of Evolution Equations, 2009zbMATH Open Web Interface contents unavailable due to conflicting licenses.
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A portable and efficient parallel code for astrophysical fluid dynamics*
, 1996 A. Malagoli +3 more
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