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

Date Issued
2017
Author(s)
DOI
Abstract
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.
Coverage
Formation, Evolution, and Survival of Massive Star Clusters
Series
Volume
vol. 12, S316
Start page
320
Conferenece
Formation, evolution, and survival of massive star clusters
Uri
Issn Identifier
1743-9213
Ads BibCode
2017IAUS..316..320C
Rights
open.access
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