Agliozzo, C.Trigilio, C.Buemi, C.Leto, P.Umana, G.Pignata, G.Phillips, N.M.Nikutta, R.Prieto, J.L.Eldridge, J.J.Bray, J.C.McClelland, L.A.S.Xiao, L.2023-08-292023-08-292016-11Proceedings of the International Astronomical Union. Open Access. Volume 12, Issue S329, Pages 69 - 73. 1 November 20161743-9213https://repositorio.unab.cl/xmlui/handle/ria/52886Indexación: Scopus.We gathered a multiwavelength dataset of two well-known LBVs. We found a com plex 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.enStars: Individual (RMC127, HR Car)Stars: Mass LossStars: WindsOutflowsThe mass-loss before the end : two luminous blue variables with a collimated stellar windArtÃculo10.1017/S1743921317003301