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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*
Affiliation:
INAF – Astronomical Observatory of Teramo, Via M. Maggini, Teramo, 64100, Italy email: [email protected]
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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.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2017 

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