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Blue Straggler Stars in Sagittarius Globular Clusters. Giovanni Carraro, ESO - Chile. Nov 06, 2012. The context:. Sgr offers a different environment to study the BS phenomenon:
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Blue Straggler Stars in Sagittarius Globular Clusters Giovanni Carraro, ESO - Chile Nov 06, 2012
The context: • Sgr offers a different environment to study the BS phenomenon: • Star clusters associated with Sgr exhibit wide variations of age, structural and dynamical properties, and metallicity.
The data: BV photometry, Danish telescope @LaSilla
The Color-Magnitude Diagrams: Arp 2 and Terzan 8 are Sgrgenuine members, NGC 5634 and Palomar 12 are stripped clusters, now floating in the MW halo.
Structural properties: cont. Sgr main body clusters
BS stars selection: Contamination taken into account in a statistical way
BS radial distribution: Not segregated Segregated Segregated Not segregated
BS specific frequency: Sgr Main Body contamination ????
BS cumulative distribution: 60 % 0.4 % 44 % 75% Anderson-Darling test
Conclusions: • The main idea of this study was to use BS as test-particle to probe the parent cluster dynamical status; • Their distribution nicely correlates with the King parameters of the parent clusters; • Special care must be taken since contamination from Sgr Main Body can complicate significantly the interpretation.
BS in Galactic Old Open Clusters • Open clusters seem to possess the largest frequency of BS (see Yazan talk) • There is a trend of having more BS at decreasing total luminosity and increasing age (De Marchi et al. 2006) • Membership is a challenge (see Javier talk)
BS in Galactic Old Open Clusters Carraro, Boffin, Ahumada, Beccari, Davies, Monaco
BS in Galactic Old Open Clusters • FLAMES (blue setup) + UVES • Multi-epoch ( typically 3 epochs) • Improving membership, improving statististics, finding pathological cases • In the middle between micro- and macro-economy