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Evolving sparse stellar populations

Published online by Cambridge University Press:  21 March 2017

Gustavo Bruzual ,
Gladis Magris C.  and
Fabiola Hernández-Pérez
Gustavo Bruzual
Affiliation:
IRyA, UNAM, Campus Morelia, Morelia, México email: g.bruzual@crya.unam.mx
Gladis Magris C.
Affiliation:
CIDA, Apartado Postal 264, Mérida, Venezuela email: magris@cida.gob.ve
Fabiola Hernández-Pérez
Affiliation:
Dpto. de Física, Grupo de Astrofísica Teórica, Fac. de Ciencias, Universidad de Los Andes, Mérida, Venezuela email: fabiolah@ula.ve
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Abstract

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We examine the role that stochastic fluctuations in the IMF and in the number of interacting binaries have on the spectro-photometric properties of sparse stellar populations as a function of age and metallicity.

Keywords

Stellar populationsGalaxy evolutionBinary evolution
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 11 , Symposium S321: Formation and Evolution of Galaxy Outskirts , March 2016 , pp. 96 - 98
Copyright
Copyright © International Astronomical Union 2017 

References

Bruzual, G. 2007, IAU Symposium No. 241 “Stellar Populations as Building Blocks of Galaxies’ eds. Vazdekis, A. and Peletier, R. F., Cambridge: Cambridge University Press, p.125 Google Scholar
Hernández-Pérez, F. & Bruzual, G. 2013, MNRAS, 431, 2612 Google Scholar
Hernández-Pérez, F. & Bruzual, G. 2014, MNRAS, 444, 2571 Google Scholar