Spectroscopic follow-up of the colliding-wind binary WR140 during the 2009 January periastron passage
Université de Montréal, Montréal, Canada
Université de Montréal, Montréal, Canada
Institut d’Astrophysique de Paris, Paris, France
Schnörringen Telescope Science Institute, Köln, Germany
Herzberg Institute of Astrophysics, Victoria, Canada
MONS pro-am collaboration
MONS pro-am collaboration
MONS pro-am collaboration
MONS pro-am collaboration
MONS pro-am collaboration
MONS pro-am collaboration
MONS pro-am collaboration
MONS pro-am collaboration
MONS pro-am collaboration
MONS pro-am collaboration
MONS pro-am collaboration
MONS pro-am collaboration
MONS pro-am collaboration
MONS pro-am collaboration
MONS pro-am collaboration
MONS pro-am collaboration
MONS pro-am collaboration
MONS pro-am collaboration
MONS pro-am collaboration
MONS pro-am collaboration
MONS pro-am collaboration
MONS pro-am collaboration
Abstract
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 (around 8 years) and eccentricity (around 0.9). 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.