A study of the blue straggler population of the old open cluster Collinder 261
M.J. Rain, G. Carraro, J.A. Ahumada, S. Villanova, H. Boffin, L., Monaco, G. Beccari

TL;DR
This study investigates the blue straggler stars in the old open cluster Collinder 261 using Gaia data and radial velocity surveys to understand their properties, distribution, and binary status, shedding light on cluster dynamics.
Contribution
It provides a comprehensive analysis of blue stragglers in Collinder 261, including their identification, binary characteristics, and spatial distribution, using combined Gaia and spectroscopic data.
Findings
Identified 53 blue stragglers in Collinder 261.
Discovered multiple binary systems among blue stragglers.
Analyzed the spatial distribution to assess mass segregation.
Abstract
Blue Stragglers are stars located in an unexpected region of the color-magnitude diagram of a stellar population, as they appear bluer and more luminous than the stars in the turnoff region. They are ubiquitous, since they have been found among Milky Way field stars, in open and globular clusters, and also in other galaxies of the Local Group. Here we present a study on the blue straggler population of the old and metal-rich open cluster Collinder 261, based on Gaia DR2 data and on a multi-epoch radial velocity survey conducted with FLAMES@VLT. We also analyze the radial distribution of the blue straggler population to probe the dynamical status of the cluster. Blue straggler candidates were identified first with Gaia DR2, according to their position on the CMD, proper motions, and parallaxes. Their radial distribution was compared with those of the main sequence, red giant, and red…
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