HD 152246 - a new high-mass triple system and its basic properties

@article{Nasseri2014HD1,
  title={HD 152246 - a new high-mass triple system and its basic properties},
  author={A. Nasseri and Rolf Chini and P. Harmanec and Pavel Mayer and J. A. Nemravov'a and T. Dembsky and Holger Lehmann and Hugues Sana and J.-B. Le Bouquin},
  journal={arXiv: Solar and Stellar Astrophysics},
  year={2014}
}
Analyses of multi-epoch, high-resolution (R ~ 50.000) optical spectra of the O-type star HD 152246 (O9 IV according to the most recent classification), complemented by a limited number of earlier published radial velocities, led to the finding that the object is a hierarchical triple system, where a close inner pair (Ba-Bb) with a slightly eccentric orbit (e = 0.11) and a period of 6.0049 days revolves in a 470-day highly eccentric orbit (e = 0.865) with another massive and brighter component A… 
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