Difference between revisions of "User:Tohline/H Book"

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==Context==
==Context==


:[http://www.vistrails.org/index.php/User:Tohline/PGE#PGE:Euler Principal Governing Equations]
:[http://www.vistrails.org/index.php/User:Tohline/PGE#Poisson:Euler Principal Governing Equations]


:Supplemental Relations
:Supplemental Relations

Revision as of 18:06, 18 January 2010


H Book title.gif


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>

Context

Principal Governing Equations
Supplemental Relations
Virial Equations

Applications

LSU Structure still.gif Structure
LSU Stable.animated.gif Stability
Minitorus.animated.gif Dynamics

Appendices