EDP Sciences
Free access
Issue A&A
Volume 482, Number 3, May II 2008
Page(s) 777 - 781
Section Galactic structure, stellar clusters, and populations
DOI http://dx.doi.org/10.1051/0004-6361:20078629
Published online 11 March 2008

A&A 482, 777-781 (2008)
DOI: 10.1051/0004-6361:20078629

Research Note

Blue straggler stars in Galactic open clusters and the effect of field star contamination

G. Carraro1, R. A. Vázquez2, and A. Moitinho3

1  ESO, Alonso de Cordova 3107, Vitacura, Santiago, Chile
    e-mail: gcarraro@eso.org
2  Facultad de Ciencias Astronómicas y Geofísicas de la UNLP, IALP-CONICET, Paseo del Bosque s/n, La Plata, Argentina
    e-mail: rvazquez@fcaglp.unlp.edu.ar
3  SIM/IDL, Faculdade de Ciências da Universidade de Lisboa, Ed. C8, Campo Grande, 1749-016 Lisboa, Portugal
    e-mail: andre@sim.ul.pt

(Received 7 September 2007 / Accepted 19 February 2008)

Context. We investigate the distribution of blue straggler stars in the field of three open star clusters.
Aims. The main purpose is to highlight the crucial role played by general Galactic disk fore-/back-ground field stars, which are often located in the same region of the color magnitude diagram as blue straggler stars.
Methods. We analyze photometry taken from the literature of 3 open clusters of intermediate/old age rich in blue straggler stars, which are projected in the direction of the Perseus arm, and study their spatial distribution and the color magnitude diagram.
Results. As expected, we find that a large portion of the blue straggler population in these clusters are simply young field stars belonging to the spiral arm. This result has important consequences on the theories of the formation and statistics of blue straggler stars in different population environments: open clusters, globular clusters, or dwarf galaxies.
Conclusions. As previously emphasized by many authors, a detailed membership analysis is mandatory before comparing the blue straggler population in star clusters to theoretical models. Moreover, these sequences of young field stars (blue plumes) are potentially powerful tracers of Galactic structure and they require further consideration.

Key words: stars: blue stragglers -- Galaxy: open clusters and associations: general -- Galaxy: disk

© ESO 2008

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Editor-in-Chief: T. Forveille
Letters Editor-in-Chief: J. Alves
Managing Editor: C. Bertout

ISSN: 0004-6361 ; e-ISSN: 1432-0746
Frequency: 12 volumes per year
Published by: EDP Sciences

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