Published in
Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S329(12), p. 402
DOI: 10.1017/s1743921317003313
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The supergiant O + O binary system HD 166734: a new study
Journal article published in 2016 by
E. Gosset,
L. Mahy 
,
Y. Damerdji,
C. Nitschelm,
H. Sana,
P. Eenens,
Y. Nazé
,
Y. Damerdji,
C. Nitschelm,
H. Sana,
P. Eenens,
Y. Nazé
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Abstract
AbstractWe present here a modern study of the radial velocity curve and of the photometric light curve of the very interesting supergiant O7.5If + O9I(f) binary system HD 166734. The physical parameters of the stars and the orbital parameters are carefully determined. We also perform the analysis of the observed X-ray light curve of this colliding-wind binary.