For the first time have been able to observe and combine a large number of observables for two SO galaxies NGC 5689 and NGC 7332, in order to apply a detailed analysis of their constituent stellar populations. We will discuss our main results from the present study of the two SO galaxies NGC 5689 and NGC 7332, on the basis of our single-age, single-metallicity stellar population models.
American Astronomical Society Meeting Abstracts #189
- Pub Date:
- January 1997