Recovering stellar population parameters via different population models and stellar libraries
Three basic ingredients are required to generate a simple stellar population (SSP) library, i.e. an initial mass function (IMF), a stellar evolution model/isochrones, and an empirical/theoretical stellar spectral library. However, there are still some uncertainties to the determination and understan...
| المؤلفون الرئيسيون: | , , , , |
|---|---|
| التنسيق: | Journal article |
| منشور في: |
Oxford University Press
2019
|