Theoretical evolutionary framework for low-mass stars in massive star clusters
Date Issued
2017
Author(s)
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
Volume
vol. 12, S316
Start page
320
Conferenece
Formation, evolution, and survival of massive star clusters
Issn Identifier
1743-9213
Ads BibCode
2017IAUS..316..320C
Rights
open.access
File(s)![Thumbnail Image]()
Loading...
Name
theoretical_evolutionary_framework_for_lowmass_stars_in_massive_star_clusters.pdf
Description
PDF editoriale
Size
1.27 MB
Format
Adobe PDF
Checksum (MD5)
7367adf7514b724fdf66136fe2c3b1b5