English

Sparse Aperture Masking of Massive Stars

Solar and Stellar Astrophysics 2011-10-03 v1 Instrumentation and Methods for Astrophysics

Abstract

We present the earliest results of our NACO/VLT sparse aperture masking (SAM) campaign to search for binarity in a sample of 60 O-type stars. We detect Delta Ks < 5 mag companions for 20-25% of our targets with separations in the range 30-100 mas (typically, 40 - 200 A.U.). Most of these companions were unknown, shedding thus new light on the multiplicity properties of massive stars in a separation and brightness regime that has been difficult to explore so far. Adding detections from other techniques (spectroscopy, interferometry, speckle, lucky imaging, AO), the fraction of O stars with at least one companion is 85% (51/60 targets). This is the largest multiplicity fraction ever found.

Keywords

Cite

@article{arxiv.1109.6654,
  title  = {Sparse Aperture Masking of Massive Stars},
  author = {H. Sana and S. Lacour and J. -B. Le Bouquin and A. de Koter and C. Moni Bidin and L. Muijres and O. Schnurr and H. Zinnecker},
  journal= {arXiv preprint arXiv:1109.6654},
  year   = {2011}
}

Comments

To appear in Four Decades of Research on Massive Stars, ASP Conf. Ser. # pages, 2 figures