Published in

Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S329(12), p. 69-73

DOI: 10.1017/s1743921317003301

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The mass-loss before the end: two luminous blue variables with a collimated stellar wind

This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

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Data provided by SHERPA/RoMEO

Abstract

AbstractWe gathered a multiwavelength dataset of two well-known LBVs. We found a complex mass-loss, with evidence of variability, such as has been seen previously. In addition, our data reveal signatures of collimated stellar winds. We propose a new scenario for these two stars where the nebula shaping is influenced by the presence of a companion star and/or fast rotation.