Theoretical model services
Theoretical spectra
Available theoretical spectra models
 
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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))

Flux typeLog(t)Z 
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