The primordial binary population II: Recovering the binary population for intermediate mass stars in Sco OB2

Details The primordial binary population II: Recovering the binary population for intermediate mass stars in Sco OB2 The primordial binary population II: Recovering the binary population for intermediate mass stars in Sco OB2

2007-07-18

arxiv.org/abs/0707.2746v1

Astronomy and Astrophysics

Astrophysics

36 pages, 11 figures, accepted by A&A

Scientific paper

10.1051/0004-6361:20077719

We characterize the binary population in the young and nearby OB association Scorpius OB2 using available observations of visual, spectroscopic, and astrometric binaries with intermediate-mass primaries. We take into account observational biases by comparing the observations with simulated observations of model associations. The available data indicate a large binary fraction (> 70% with 3sigma confidence), with a large probability that all intermediate mass stars in Sco OB2 are part of a binary system. The binary systems have a mass ratio distribution of the form f(q) ~ q^-0.4. Sco OB2 has a semi-major axis distribution of the form f(log a) ~ constant (Opik's law), in the range 5-5e6 Rsun. The log-normal period distribution of Duquennoy & Mayor results in too few spectroscopic binaries, even if the model binary fraction is 100%. Sco OB2 is a young association with a low stellar density; its current population is expected to be very similar to the primordial population. The fact that practically all stars in Sco OB2 are part of a binary (or multiple) system demonstrates that multiplicity is a fundamental factor in the star formation process, at least for intermediate mass stars.

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