Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S329(12), p. 69-73, 2016
DOI: 10.1017/s1743921317003301
Full text: Unavailable
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.