In:
Proceedings of the International Astronomical Union, Cambridge University Press (CUP), Vol. 2, No. S238 ( 2006-08), p. 331-332
Abstract:
We have developed an orbit-based method for constructing triaxial models of elliptical galaxies, which fit their observed surface brightness and kinematics (van den Bosch et al ). We have tested this extended Schwarzschild method (1979) against analytical models with general distribution functions (DF) and find that we can recover the DF (van de Ven et al ). Here, we present a model of NGC 4365.
Type of Medium:
Online Resource
ISSN:
1743-9213
,
1743-9221
DOI:
10.1017/S1743921307005303
Language:
English
Publisher:
Cambridge University Press (CUP)
Publication Date:
2006
detail.hit.zdb_id:
2170724-8
SSG:
16,12
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