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Дата изменения: Wed Feb 12 19:27:07 1997
Дата индексирования: Tue Oct 2 00:47:33 2012
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Поисковые слова: ngc 5128
The Isothermal Sphere

This is mostly a blackboard lecture and derivation today.

Go here for a quasi-html version

Basic Physical Points (from Binney and Tremaine 1987:)

The structure of an isothermal self-gravitating sphere of gas is identical to a collionless systems of stars whose phase-space density can be described by a Maxwell-Boltzmann distribution.

We also make use of Jeans Theorem:

Any steady-state solution of the collisionless Boltzmann equation depends on the phase-space density coordinates only through integrals of motion in the galactic potential. Furthermore, any function of the integrals yields a steady-state solution of the collisionless Boltzmann equation.


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