Seminar
    Thinking about stellar populations modeling
Resumen
The basis of stellar population modeling was established around 40 years ago somehow
 optimized to the technical facilities and observational data available at that epoch. Since then,
 it has been used extensively in astronomy and there has been great improvements relating
 their associated ingredients in concordance with the development of more powerful computational
 and observational facilities.
 However, there has been no similar improvements in the understanding about what is
 actually modeling neither in improve the modeling itself to include the current technical advances
 to obtain more accurate result in the physical inferences obtained from them.
 In this talk I present some advances in the subject of stellar
 population modeling and how to take advantage of current facilities to obtain more robust
 and accurate inferences from stellar systems at different scales
 covering the continuum between fully resolved populations to fully unresolved ones in a unified framework.
Sobre la charla
IAA
 
       
    
star clusters, science, stellar content, Spectral energy distribution, Hertzsprung-Russell diagram, Initial Mass Function, luminosity function, mass function, stellar populations
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