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Young stellar populations in several photometric systems

Published online by Cambridge University Press:  26 May 2016

Léo Girardi ,
Gianpaolo Bertelli ,
Cesare Chiosi  and
Paola Marigo
Léo Girardi
Affiliation:
Osservatorio Astronomico di Trieste, Via G.B. Tiepolo 11, I-34131 Trieste, Italia
Gianpaolo Bertelli
Affiliation:
Consiglio Nazionale delle Richerche, Dipartimento di Astronomia, Università di Padova, Vicolo dell'Osservatorio 5, I-35122 Padova, Italia
Cesare Chiosi
Affiliation:
Dipartimento di Astronomia, Università di Padova, Vicolo dell'Osservatorio 5, I-35122 Padova, Italia
Paola Marigo
Affiliation:
Dipartimento di Astronomia, Università di Padova, Vicolo dell'Osservatorio 5, I-35122 Padova, Italia

Abstract

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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.

Type
Part 3. Location and Distribution of Massive Stars
Information
Symposium - International Astronomical Union , Volume 212: A Massive Star Odyssey: From Main Sequence to Supernova , 2003 , pp. 551 - 552
Copyright
Copyright © Astronomical Society of the Pacific 2003 

References

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