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...
| Egile nagusia: | |
|---|---|
| Formatua: | Journal article |
| Argitaratua: |
Oxford University Press
2019
|