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

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dc.contributor.authorAgliozzo, C.
dc.contributor.authorTrigilio, C.
dc.contributor.authorBuemi, C.
dc.contributor.authorLeto, P.
dc.contributor.authorUmana, G.
dc.contributor.authorPignata, G.
dc.contributor.authorPhillips, N.M.
dc.contributor.authorNikutta, R.
dc.contributor.authorPrieto, J.L.
dc.contributor.authorEldridge, J.J.
dc.contributor.authorBray, J.C.
dc.contributor.authorMcClelland, L.A.S.
dc.contributor.authorXiao, L.
dc.date.accessioned2023-08-29T15:00:29Z
dc.date.available2023-08-29T15:00:29Z
dc.date.issued2016-11
dc.descriptionIndexación: Scopus.es
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.es
dc.description.urihttps://www-cambridge-org.recursosbiblioteca.unab.cl/core/journals/proceedings-of-the-international-astronomical-union/article/massloss-before-the-end-two-luminous-blue-variables-with-a-collimated-stellar-wind/6A0233B38CAA4C72B40EF6419D07FD7E
dc.identifier.citationProceedings of the International Astronomical Union. Open Access. Volume 12, Issue S329, Pages 69 - 73. 1 November 2016es
dc.identifier.doi10.1017/S1743921317003301
dc.identifier.issn1743-9213
dc.identifier.urihttps://repositorio.unab.cl/xmlui/handle/ria/52886
dc.language.isoenes
dc.publisherCambridge University Presses
dc.subjectStars: Individual (RMC127, HR Car)es
dc.subjectStars: Mass Losses
dc.subjectStars: Windses
dc.subjectOutflowses
dc.titleThe mass-loss before the end : two luminous blue variables with a collimated stellar windes
dc.typeArtículoes
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