Results 191 to 200 of about 36,417 (233)

Primordial black holes and their gravitational-wave signatures. [PDF]

open access: yesLiving Rev Relativ
Bagui E   +20 more
europepmc   +1 more source

Field-particle energy transfer during chorus emissions in space. [PDF]

open access: yesNature
Liu CM   +8 more
europepmc   +1 more source

Stellar Astrophysical Fluid Dynamics

2003
In all phases of the life of a star, hydrodynamical processes play a major role. This volume gives a comprehensive overview of the state of knowledge in stellar astrophysical fluid dynamics, and its publication marked the 60th birthday of Douglas Gough, Professor of Theoretical Physics at the University of Cambridge and leading contributor to stellar ...
Thompson, M.J.   +1 more
openaire   +3 more sources

Computational Astrophysical Fluid Dynamics

Astrophysics and Space Science, 2000
zbMATH Open Web Interface contents unavailable due to conflicting licenses.
openaire   +1 more source

Numerical Fluid Dynamics in Astrophysics

2009
The 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
openaire   +2 more sources

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
openaire   +1 more source

Topics in Astrophysical Fluid Dynamics

2006
This 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,
openaire   +2 more sources

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