Published in
Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S329(12), p. 445-445, 2016
DOI: 10.1017/s1743921317001995
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The formation of Wolf-Rayet stars in the SMC is not dominated by mass transfer
Journal article published in 2016 by
Tomer Shenar 
,
R. Hainich,
H. Todt,
A. Sander,
W.-R. Hamann,
A. Moffat,
J. J. Eldridge,
H. Pablo,
L. Oskinova,
N. Richardson
,
R. Hainich,
H. Todt,
A. Sander,
W.-R. Hamann,
A. Moffat,
J. J. Eldridge,
H. Pablo,
L. Oskinova,
N. Richardson
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Abstract
AbstractWe analyzed spectra of all Wolf-Rayet stars in the Small Magellanic Cloud (SMC). We find that, unlike predicted, mass-transfer in binaries is not needed to explain their formation.
