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The formation of Wolf-Rayet stars in the SMC is not dominated by mass transfer
Published online by Cambridge University Press: 28 July 2017
Abstract
We 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.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 12 , Symposium S329: The Lives and Death-Throes of Massive Stars , November 2016 , pp. 445
- Copyright
- Copyright © International Astronomical Union 2017