Difference between revisions of "User:Tohline/H Book"
m (→Context: point to Poisson equation instead of Euler) |
m (→Context: fix previous) |
||
| Line 20: | Line 20: | ||
==Context== | ==Context== | ||
:[http://www.vistrails.org/index.php/User:Tohline/PGE#Poisson | :[http://www.vistrails.org/index.php/User:Tohline/PGE#PGE:Poisson Principal Governing Equations] | ||
:Supplemental Relations | :Supplemental Relations | ||
Revision as of 18:07, 18 January 2010
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
- Supplemental Relations
- Virial Equations
Applications
Structure
Stability
Dynamics
