Difference between revisions of "User:Tohline/H Book"
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==Applications== | ==Applications== | ||
: | # <font color="darkblue">'''Non-rotating, uniform-density sphere:'''</font> | ||
: [[Image:Minitorus.animated.gif|74px]] | <div align="right"> | ||
<table border=1 cellpadding=8 width="95%"> | |||
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<td width="10%" align="center" valign="top"> | |||
Structure<br /> | |||
[[Image:LSU_Structure_still.gif|74px]] | |||
</td> | |||
<td align="left" valign="top"> | |||
<font color="red">SUMMARY:</font> The equilibrium structure of a self-gravitating, non-rotating, uniform-density sphere can be described analytically. | |||
</td> | |||
</tr> | |||
<tr> | |||
<td width="10%" align="center" valign="top"> | |||
Stability<br /> | |||
[[Image:LSU_Stable.animated.gif|74px]] | |||
</td> | |||
<td align="left" valign="top"> | |||
<font color="red">SUMMARY:</font> The equilibrium structure of a self-gravitating, non-rotating, uniform-density sphere can be described analytically. | |||
</td> | |||
</tr> | |||
<tr> | |||
<td width="10%" align="center" valign="top"> | |||
Dynamics<br /> | |||
[[Image:Minitorus.animated.gif|74px]] | |||
</td> | |||
<td align="left" valign="top"> | |||
<font color="red">SUMMARY:</font> The equilibrium structure of a self-gravitating, non-rotating, uniform-density sphere can be described analytically. | |||
</td> | |||
</tr> | |||
</table> | |||
</div> | |||
==Appendices== | ==Appendices== | ||
{{LSU_HBook_footer}} | {{LSU_HBook_footer}} | ||
Revision as of 03:11, 31 January 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>
Context
- Virial Equations
Applications
- Non-rotating, uniform-density sphere:
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Structure |
SUMMARY: The equilibrium structure of a self-gravitating, non-rotating, uniform-density sphere can be described analytically. |
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Stability |
SUMMARY: The equilibrium structure of a self-gravitating, non-rotating, uniform-density sphere can be described analytically. |
|
Dynamics |
SUMMARY: The equilibrium structure of a self-gravitating, non-rotating, uniform-density sphere can be described analytically. |
Appendices
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© 2014 - 2021 by Joel E. Tohline |