Sco OB2 intermediate-mass stars (Kouwenhoven+, 2007)

Details Sco OB2 intermediate-mass stars (Kouwenhoven+, 2007) Sco OB2 intermediate-mass stars (Kouwenhoven+, 2007)

Mar 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007ycat..34640581k&link_type=abstract

VizieR On-line Data Catalog: J/A+A/464/581. Originally published in: 2007A&A...464..581K

Physics

Clusters: Open, Stars: Double And Multiple, Photometry: Infrared

Scientific paper

We present JHK observations of 22 intermediate-mass stars in Sco OB2, obtained with NACO. This survey was performed to determine the status of (sub)stellar candidate companions of Sco OB2 member stars of spectral type A and late-B. The distinction between companions and background stars is made on the basis of a comparison to isochrones and additional statistical arguments. We include in our sample a subset of 9 targets with multi-color ADONIS observations from Kouwenhoven et al. (2005, Cat. ). We reanalyse the total sample (i.e. NACO and ADONIS) and conclude that of the 176 secondaries, 25 are physical companions, 55 are candidate companions, and 96 are background stars. Although we are sensitive (and complete) to brown dwarf companions as faint as K=14mag in the semi-major axis range 130-520AU, we detect only one, corresponding to a brown dwarf companion fraction of 0.5% (M>30MJupiter). However, the number of brown dwarfs is consistent with an extrapolation of the (stellar) companion mass distribution into the brown dwarf regime. This indicates that the physical mechanism for the formation of brown dwarf companions around intermediate mass stars is similar to that of stellar companions, and that the embryo ejection mechanism does not need to be invoked in order to explain the small number of brown dwarf companions among intermediate mass stars in Sco OB2.
(5 data files).

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