Visual binaries among high-mass stars - An adaptive optics survey of OB stars in the NGC 6611 cluster

Abstract

We have searched for visual binaries with projected separations in the range 200-3000 AU (0.1"-1.5") among a sample of 96 stars in the massive young NGC 6611 cluster, 60 of them being subsequently identified as high probability cluster members of mainly OB spectral type. This is the first visual binary survey among such a large and homogeneous sample of high-mass stars. We find an uncorrected binary frequency of 18+/-6% over the surveyed separation range. Considering only binaries with mass ratios q>0.1, we find that OB stars in NGC 6611 host more companions than solar-type field stars. We derive mass ratios for the detected binaries from their near-infrared flux ratios and conclude that about half of the detected binaries have q<0.2, which does not contradict the assumption that companion masses are randomly drawn from the initial mass function. There is no evidence in our sample that wide-binary properties depend upon the mass of the primary star. The high frequency of massive binaries in a cluster as rich as NGC 6611 and the lack of a strong mass dependence of their properties are difficult to reconcile with the scenario whereby massive stars form as the result of mergers of smaller stars. The canonical protostellar accretion scenario together with cloud fragmentation, on the other hand, can naturally explain most of the observed binary properties, although the very high stellar density in the protocluster is likely to require significant modification to that picture as well.

arXiv commentAccepted for publication in A&A, LaTeX2e, 15 pages, 5 embedded figures

References in corpus (9)

• On the Formation of Massive Stars
• The Formation of a Bound Star Cluster: From the Orion Nebula Cluster to the Pleiades
• Structure and Evolution of the Envelopes of Deeply Embedded Massive Young Stars
• Formation of massive stars by growing accretion rate
• Star Cluster Evolution, Dynamical Age Estimation and the Kinematical Signature of Star Formation
• Binary stars in young clusters: models versus observations of the Trapezium Cluster
• Wide binaries in the Orion Nebula Cluster
• Search for low-mass PMS companions around X-ray selected late B stars
• The formation and evolution of binary systems. III. Low-mass binaries in the Praesepe cluster

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• The stellar and sub-stellar IMF of simple and composite populations
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• The VLT-FLAMES Survey of Massive Stars: Observations in the Galactic Clusters NGC 3293, NGC 4755 and NGC 6611
• An Updated Look at Binary Characteristics of Massive Stars in the Cygnus OB2 Association
• Multiple protostellar systems. I. A deep near infrared survey of Taurus and Ophiuchus protostellar objects
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• The Close Binary Properties of Massive Stars in the Milky Way and Low-Metallicity Magellanic Clouds
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• Observational properties of visual binaries as modelled using a synthetic catalogue, I: For visual apparent magnitudes $m_v<15$
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