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| ==Applications== | | ==Applications== |
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| # <font color="darkblue">'''Non-rotating, uniform-density sphere:'''</font> | | # <font color="darkblue">'''[http://www.vistrails.org/index.php/User:Tohline/SphericallySymmetricStructures Spherically Symmetric Structures]:'''</font> |
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| Structure<br />
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| [[Image:LSU_Structure_still.gif|74px]] | |
| </td>
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| <font color="red">SUMMARY:</font> The equilibrium structure of a self-gravitating, non-rotating, uniform-density sphere can be described analytically. The equilibrium structure of a self-gravitating, non-rotating, uniform-density sphere can be described analytically. The equilibrium structure of a self-gravitating, non-rotating, uniform-density sphere can be described analytically. The equilibrium structure of a self-gravitating, non-rotating, uniform-density sphere can be described analytically. The equilibrium structure of a self-gravitating, non-rotating, uniform-density sphere can be described analytically. The equilibrium structure of a self-gravitating, non-rotating, uniform-density sphere can be described analytically. The equilibrium structure of a self-gravitating, non-rotating, uniform-density sphere can be described analytically.
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| <td width="10%" align="center" valign="top">
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| Stability<br />
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| [[Image:LSU_Stable.animated.gif|74px]]
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| </td>
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| <td align="left" valign="top">
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| <font color="red">SUMMARY:</font> The equilibrium structure of a self-gravitating, non-rotating, uniform-density sphere can be described analytically. The equilibrium structure of a self-gravitating, non-rotating, uniform-density sphere can be described analytically. The equilibrium structure of a self-gravitating, non-rotating, uniform-density sphere can be described analytically. The equilibrium structure of a self-gravitating, non-rotating, uniform-density sphere can be described analytically. The equilibrium structure of a self-gravitating, non-rotating, uniform-density sphere can be described analytically. The equilibrium structure of a self-gravitating, non-rotating, uniform-density sphere can be described analytically. The equilibrium structure of a self-gravitating, non-rotating, uniform-density sphere can be described analytically.
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| <td width="10%" align="center" valign="top">
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| Dynamics<br />
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| [[Image:Minitorus.animated.gif|74px]]
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| </td>
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| <td align="left" valign="top">
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| <font color="red">SUMMARY:</font> The equilibrium structure of a self-gravitating, non-rotating, uniform-density sphere can be described analytically. The equilibrium structure of a self-gravitating, non-rotating, uniform-density sphere can be described analytically. The equilibrium structure of a self-gravitating, non-rotating, uniform-density sphere can be described analytically. The equilibrium structure of a self-gravitating, non-rotating, uniform-density sphere can be described analytically. The equilibrium structure of a self-gravitating, non-rotating, uniform-density sphere can be described analytically. The equilibrium structure of a self-gravitating, non-rotating, uniform-density sphere can be described analytically. The equilibrium structure of a self-gravitating, non-rotating, uniform-density sphere can be described analytically.
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| </td>
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| </tr>
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| </table>
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| </div>
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| ==Appendices== | | ==Appendices== |
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| {{LSU_HBook_footer}} | | {{LSU_HBook_footer}} |
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
- Spherically Symmetric Structures:
Appendices
