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Theoretical evolutionary framework for low-mass stars in massive star clusters

Published online by Cambridge University Press:  31 March 2017

Santi Cassisi
Santi Cassisi*
Affiliation:
INAF – Astronomical Observatory of Teramo, Via M. Maggini, Teramo, 64100, Italy email: cassisi@oa-teramo.inaf.it
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Abstract

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Recent spectroscopic and photometric surveys of Galactic Globular Clusters have shown that these stellar systems host distinct sub-populations of stars characterised by peculiar chemical patterns. In the following we wish to address the issue of how these specific chemical patterns affect both the structural and evolutionary properties of stars as well as their spectral energy distribution. The implications of these effects on the photometric appearance of multiple stellar populations in different photometric planes are also briefly discussed.

Keywords

stars: Population IIstars: low-massstars: interiorsstars: evolution
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 12 , Symposium S316: Formation, evolution, and survival of massive star clusters , August 2015 , pp. 320 - 327
Copyright
Copyright © International Astronomical Union 2017 

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