The WR 140 periastron passage 2009: first results from MONS and other   optical sources
  We present the results from the spectroscopic follow-up of WR140 (WC7 + O4-5) during its last periastron passage in January 2009. This object is known as the archetype of colliding wind binaries and has a relatively large period (~ 8 years) and eccentricity (~ 0.89). We provide updated values for the orbital parameters, new estimates for the WR and O star masses and new constraints on the mass-loss rates. 
R. Fahed, A. F. J. Moffat, J. Zorec, T. Eversberg, A. N. Chen\'e, F.   Alves, W. Arnold, T. Bergmann, L. F. Gouveia Carreira...
astro-ph.SR