- Startpagina tijdschrift
- Volume 80 - Année 2011
- Spectroscopic follow-up of the colliding-wind binary WR140 during the 2009 January periastron passage
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Spectroscopic follow-up of the colliding-wind binary WR140 during the 2009 January periastron passage
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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.
Om dit artikel te citeren:
Over : R. Fahed
Université de Montréal, Montréal, Canada
Over : A. F. J. Moffat
Université de Montréal, Montréal, Canada
Over : J. Zorec
Institut d’Astrophysique de Paris, Paris, France
Over : T. Eversberg
Schnörringen Telescope Science Institute, Köln, Germany
Over : A. N. Chené
Herzberg Institute of Astrophysics, Victoria, Canada
Over : F. Alves
MONS pro-am collaboration
Over : W. Arnold
MONS pro-am collaboration
Over : T. Bergmann
MONS pro-am collaboration
Over : L. F. Gouveia Carreira
MONS pro-am collaboration
Over : F. Marques Dias
MONS pro-am collaboration
Over : A. Fernando
MONS pro-am collaboration
Over : J. Sanchez Gallego
MONS pro-am collaboration
Over : T. Hunger
MONS pro-am collaboration
Over : J. Knapen
MONS pro-am collaboration
Over : R. Leadbeater
MONS pro-am collaboration
Over : T. Morel
MONS pro-am collaboration
Over : G. Rauw
MONS pro-am collaboration
Over : N. Reinecke
MONS pro-am collaboration
Over : J. Ribeiro
MONS pro-am collaboration
Over : N. Romeo
MONS pro-am collaboration
Over : E. M. dos Santos
MONS pro-am collaboration
Over : L. Schanne
MONS pro-am collaboration
Over : O. Stahl
MONS pro-am collaboration
Over : Ba. Stober
MONS pro-am collaboration
Over : Be. Stober
MONS pro-am collaboration
Over : N. G. Correia Viegas
MONS pro-am collaboration
Over : K. Vollmann
MONS pro-am collaboration