Orbit-superposition models of discrete, incomplete stellar kinematics: application to the Galactic centre
We present a method for fitting orbit-superposition ("Schwarzschild") models to the kinematics of discrete stellar systems when the available stellar sample is not complete, but has been filtered by a known selection function. As an example, we apply it to Fritz et al.'s kinematics of...
Autor principal: | Magorrian, J |
---|---|
Format: | Journal article |
Publicat: |
Oxford University Press
2019
|
Ítems similars
-
Kinematical signatures of hidden stellar discs
per: Magorrian, J
Publicat: (1999) -
Three-dimensional Keplerian orbit-superposition models of the nucleus of
M31
per: Brown, C, et al.
Publicat: (2013) -
Constraining black hole masses from stellar kinematics by summing over all possible distribution functions
per: Magorrian, J
Publicat: (2006) -
The population of Galactic Centre filaments - III. Candidate radio and stellar sources
per: Yusef-Zadeh, F, et al.
Publicat: (2022) -
The impact of AGN on stellar kinematics and orbits in simulated massive galaxies
per: Frigo, M, et al.
Publicat: (2019)