Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S316(12), p. 320-327
DOI: 10.1017/s1743921315008881
Full text: Unavailable
AbstractRecent 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.