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Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S238(2), p. 331-332, 2006

DOI: 10.1017/s1743921307005303

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Triaxial orbit-based model of NGC 4365

Journal article published in 2006 by Remco C. E. van den Bosch, Glenn van de Ven ORCID, Michele Cappellari, P. Tim de Zeeuw
This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

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Abstract

AbstractWe 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.

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