POPSTAR with Salpeter IMF (2)
PopStar Evolutionary synthesis models. Using IMF from Salpeter (1955) with m=(0.15-100)Msun.
This grid of Single Stellar Populations covers a wide range in both, age and metallicity. The models use the most recent evolutionary tracks together with the use of new NLTE atmosphere models. (Mollá, García-Vargas & Bressan (2009))
- Molla, M.; Garcia-Vargas, M. L.; Bressan, A., 2009, MNRAS, 398,451
PopStar I: evolutionary synthesis model description.
- Salpeter E.E., 1955, ApJ 121, 161.
The Luminosity Function and Stellar Evolution