Difference between revisions of "User:Tohline/H Book"
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** Zero-temperature White Dwarf | ** Zero-temperature White Dwarf | ||
** Isothermal sphere | ** Isothermal sphere | ||
===Stability:=== | ===Stability:=== | ||
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** [[User:Tohline/SSC/Polytropes|Polytropes]] | ** [[User:Tohline/SSC/Polytropes|Polytropes]] | ||
===<font color="darkblue">'''[[User:Tohline/SphericallySymmetricConfigurations|Dynamics]]:'''</font>=== | |||
==Two-Dimensional Configurations== | |||
* Introduction | |||
===Structure:=== | |||
* <font color="darkblue">'''Solution Strategies'''</font> | |||
* Example Solutions: | |||
** Maclaurin Spheroids | |||
** [[User:Tohline/Apps/Korycansky_Papaloizou_1996|Infinitesimally Thin, Nonaxisymmetric Disk]] | |||
===Stability:=== | |||
===Dynamics:=== | |||
==Three-Dimensional Configurations== | |||
===<font color="darkblue">'''[[User:Tohline/ | * Introduction | ||
===Structure:=== | |||
* <font color="darkblue">'''Solution Strategies'''</font> | |||
* Example Solutions: | |||
** Ellipsoidal Figures of Equilibrium | |||
** [[User:Tohline/Apps/RiemannEllipsoids_Compressible|Compressible Analogs of Riemann Ellipsoids]] | |||
===Stability:=== | |||
===Dynamics:=== | |||
=Appendices= | =Appendices= | ||
{{LSU_HBook_footer}} | {{LSU_HBook_footer}} |
Revision as of 17:47, 21 March 2010
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Preface from the original version of this HyperText Book (H_Book):
November 18, 1994
Much of our present, basic understanding of the structure, stability, and dynamical evolution of individual stars, short-period binary star systems, and the gaseous disks that are associated with numerous types of stellar systems (including galaxies) is derived from an examination of the behavior of a specific set of coupled, partial differential equations. These equations — most of which also are heavily utilized in studies of continuum flows in terrestrial environments — are thought to govern the underlying physics of all macroscopic "fluid" systems in astronomy. Although relatively simple in form, they prove to be very rich in nature... <more>
Pictorial Table of Contents
Context
- Principal Governing Equations
- Continuity Equation
- Euler Equation
- <math>1^\mathrm{st}</math> Law of Thermodynamics
- Poisson Equation
- Virial Equations
Applications
Spherically Symmetric Configurations
Structure:
- Solution Strategies
- Example Solutions:
- Uniform-density sphere
- Polytropes
- Zero-temperature White Dwarf
- Isothermal sphere
Stability:
- Solution Strategy
- Example Solutions:
Dynamics:
Two-Dimensional Configurations
- Introduction
Structure:
- Solution Strategies
- Example Solutions:
- Maclaurin Spheroids
- Infinitesimally Thin, Nonaxisymmetric Disk
Stability:
Dynamics:
Three-Dimensional Configurations
- Introduction
Structure:
- Solution Strategies
- Example Solutions:
- Ellipsoidal Figures of Equilibrium
- Compressible Analogs of Riemann Ellipsoids
Stability:
Dynamics:
Appendices
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