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

dc.creatorAgliozzo, C.
dc.creatorTrigilio, C.
dc.creatorBuemi, C.
dc.creatorLeto, P.
dc.creatorUmana, G.
dc.creatorPignata, G.
dc.creatorPhillips, N.M.
dc.creatorNikutta, R.
dc.creatorPrieto, J.L.
dc.creatorEldridge, J.J.
dc.creatorBray, J.C.
dc.creatorMcClelland, L.A.S.
dc.creatorXiao, L.
dc.date.accessioned2023-08-29T15:00:29Z
dc.date.accessioned2024-05-02T15:05:37Z
dc.date.available2023-08-29T15:00:29Z
dc.date.available2024-05-02T15:05:37Z
dc.date.created2023-08-29T15:00:29Z
dc.date.issued2016-11
dc.identifierProceedings of the International Astronomical Union. Open Access. Volume 12, Issue S329, Pages 69 - 73. 1 November 2016
dc.identifier1743-9213
dc.identifierhttps://repositorio.unab.cl/xmlui/handle/ria/52886
dc.identifier10.1017/S1743921317003301
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/9262301
dc.description.abstractWe 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.
dc.languageen
dc.publisherCambridge University Press
dc.subjectStars: Individual (RMC127, HR Car)
dc.subjectStars: Mass Loss
dc.subjectStars: Winds
dc.subjectOutflows
dc.titleThe mass-loss before the end : two luminous blue variables with a collimated stellar wind
dc.typeArtículo


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