Volume 421, Issue 2 pp. 960-970

Structural parameters and blue stragglers in Sagittarius dwarf spheroidal galaxy globular clusters

Ricardo Salinas

Corresponding Author

Ricardo Salinas

Finnish Centre for Astronomy with ESO (FINCA), University of Turku, Väisäläntie 20, FI-21500 Piikkiö, Finland

Based on data collected at the Danish Telescope at the ESO La Silla Observatory.

E-mail: [email protected]

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Lucie Jílková

Lucie Jílková

European Southern Observatory, Alonso de Córdova 3107, Casilla 19001, Santiago 19, Chile

Department of Theoretical Physics and Astrophysics, Faculty of Science, Masaryk University, Kotlářská 2, CZ-611 37 Brno, Czech Republic

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Giovanni Carraro

Giovanni Carraro

European Southern Observatory, Alonso de Córdova 3107, Casilla 19001, Santiago 19, Chile

Dipartimento di Astronomia, Universitá di Padova, Vicolo Osservatorio 5, I-35122 Padova, Italy

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Márcio Catelan

Márcio Catelan

Departamento de Astronomía y Astrofísica, Pontificia Universidad Católica de Chile, Av. Vicuña Mackenna 4860, 782-0436 Macul, Santiago, Chile

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Pía Amigo

Pía Amigo

Departamento de Astronomía y Astrofísica, Pontificia Universidad Católica de Chile, Av. Vicuña Mackenna 4860, 782-0436 Macul, Santiago, Chile

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First published: 29 February 2012

ABSTRACT

We present BV photometry of four Sagittarius dwarf spheroidal galaxy globular clusters: Arp 2, NGC 5634, Palomar 12 and Terzan 8, obtained with the Danish Telescope at ESO La Silla. We measure the structural parameters of the clusters using a King profile fitting, obtaining the first reliable measurements of the tidal radius of Arp 2 and Terzan 8. These two clusters are remarkably extended and with low concentrations; with a concentration of only c= 0.41 ± 0.02, Terzan 8 is less concentrated than any cluster in our Galaxy.

Blue stragglers are identified in the four clusters, and their spatial distribution is compared to those of horizontal branch and red giant branch stars. The blue straggler properties do not provide evidence of mass segregation in Terzan 8, while Arp 2 probably shares the same status, although with less confidence. In the case of NGC 5634 and Palomar 12, blue stragglers are significantly less populous, and their analysis suggests that the two clusters have probably undergone mass segregation.

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