An Introduction to Astrophysical Hydrodynamics
This book is an introduction to astrophysical hydrodynamics for both astronomy and physics students. It provides a comprehensive and unified view of the general problems associated with fluids in a cosmic context, with a discussion of fluid dynamics and plasma physics. It is the only book on hydrodynamics that addresses the astrophysical context. Researchers and students will find this work to be an exceptional reference. Contents include chapters on irrotational and rotational flows, turbulence, magnetohydrodynamics, and instabilities.
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acceleration accretion disk adiabatic Alfvén angular momentum approximation assume Astron Astrophys astrophysical atmosphere blast wave boundary layer components compressible conﬁguration conservation constant continuity equation convection deﬁned deﬁnition density depends derived diffusion discussion dissipation distribution function dynamical effects emission energy equations of motion equilibrium evolution expanding ﬁnal ﬁnd ﬁnite ﬁrst ﬁxed ﬂow ﬂuctuations ﬂuid ﬂux frequency front galactic galaxy gravitational H II region heat hydrodynamic incompressible instability integral interstellar medium ionization isothermal kinetic line proﬁle luminosity Mach number magnetic ﬁeld main sequence mass loss mean mechanism molecular clouds observed optical depth optically thin outﬂow particles perturbation photons physical plasma polytropic potential pressure problem radiation radiative radius reﬂected result rotation scale shear shock solution sound speed speciﬁc spectrum spherical star stellar wind structure supersonic surface temperature tensor term theorem thermal tion turbulence vanishes variables velocity ﬁeld virial theorem viscosity vorticity