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Young stellar populations in several photometric systems
Published online by Cambridge University Press: 26 May 2016
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.
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- Part 3. Location and Distribution of Massive Stars
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- Copyright © Astronomical Society of the Pacific 2003
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