We report on two recent improvements to the library of stellar models from Padova. (i) A new set of massive stellar models has been computed for the metallicity Z = 0.001, thus filling an important gap in the previously existing library. (ii) We started a project aiming to convert the complete set of isochrones into a wide variety of photometric systems.
Young stellar populations in several photometric systems
CHIOSI, CESARE;MARIGO, PAOLA
2003
Abstract
We report on two recent improvements to the library of stellar models from Padova. (i) A new set of massive stellar models has been computed for the metallicity Z = 0.001, thus filling an important gap in the previously existing library. (ii) We started a project aiming to convert the complete set of isochrones into a wide variety of photometric systems.File in questo prodotto:
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