Abstract
We take a sample of 24 elliptical and lenticular galaxies previously analysed by the SAURON project using three integral dynamical models created with Schwarzschild method, and re-analyse them using the made-to-measure (M2M) method of dynamical modelling. We obtain good agreement between the two methods in determining the dynamical mass-to-light ratios (M/L values) for the galaxies with over 80 percent of ratios differing by
| Original language | English |
|---|---|
| Pages (from-to) | 2580-2592 |
| Number of pages | 12 |
| Journal | Monthly Notices of the Royal Astronomical Society |
| Volume | 421 |
| Issue number | 3 |
| DOIs | |
| Publication status | Published - Apr 2012 |
Keywords
- Galaxies: elliptical and lenticular, cD
- Galaxies: kinematics and dynamics
- Galaxies: structure
- Methods: numerical