Integrals of Motion in an Elliptical Galaxy Model
1987 ◽
Vol 127
◽
pp. 485-486
Keyword(s):
The structure of a galaxy model is described completely by its phase–space distribution function f. By Jeans' Theorem f can be written as a function of the integrals of motion admitted by the potential of the model. Various independent combinations of the integrals may be used as arguments of f; in many cases the action integrals are to be preferred. For a general N–body model, these can be obtained by numerical integration and subsequent spectral decomposition of each orbit (Binney and Spergel 1984).
1998 ◽
Vol 235
(1-3)
◽
pp. 213-225
◽
Keyword(s):
Keyword(s):
2012 ◽
Vol 10
(H16)
◽
pp. 349-349
Keyword(s):
2000 ◽
Vol 17
(12)
◽
pp. 2464
◽
Keyword(s):
1988 ◽
Vol 61
(5)
◽
pp. 503-506
◽
Keyword(s):
Keyword(s):
1985 ◽
Vol 83
(7)
◽
pp. 3491-3499
◽
1965 ◽
Vol 6
(12)
◽
pp. 1913-1915
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