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dc.contributor.authorBuemi, C.S.
dc.contributor.authorTrigilio, C.
dc.contributor.authorLeto, P.
dc.contributor.authorUmana, G.
dc.contributor.authorIngallinera, A.
dc.contributor.authorCavallaro, F.
dc.contributor.authorCerrigone, L.
dc.contributor.authorAgliozzo, C.
dc.contributor.authorBufano, F.
dc.contributor.authorRiggi, S.
dc.contributor.authorMolinari, S.
dc.contributor.authorSchillirò, F.
dc.date.accessioned2017-09-14T20:03:34Z
dc.date.available2017-09-14T20:03:34Z
dc.date.issued2016-12
dc.identifier.citationMonthly Notices of the Royal Astronomical Society, Volume 465, Issue 4, 11 March 2017, Pages 4147–4158es_CL
dc.identifier.issn1365-2966
dc.identifier.issn0035-8711
dc.identifier.otherhttps://doi.org/10.1093/mnras/stw3074
dc.identifier.urihttp://repositorio.unab.cl/xmlui/handle/ria/4245
dc.descriptionIndexación: Web of Science; Scopus.es_CL
dc.description.abstractWe present a multiwavelength study of the Galactic luminous blue variable HR Carinae, based on new high-resolution mid-infrared (IR) and radio images obtained with the Very Large Telescope (VLT) and the Australia Telescope Compact Array (ATCA), which have been complemented by far-infrared Herschel-Photodetector Array Camera and Spectrometer (PACS) observations and ATCA archive data. The Herschel images reveal the large-scale distribution of the dusty emitting nebula, which extends mainly to the north-east direction, up to 70 arcsec from the central star, and is oriented along the direction of the space motion of the star. In the mid-infrared images, the brightness distribution is characterized by two arcshaped structures, tracing an inner envelope surrounding the central star more closely. At radio wavelengths, the ionized gas emission lies on the opposite side of the cold dust with respect to the position of the star, as if the ionized front were confined by the surrounding medium in the north-south direction. Comparison with previous data indicates significant changes in the radio nebula morphology and in the mass-loss rate from the central star, which has increased from 6.1 × 10-6M⊙ yr-1 in 1994-1995 to 1.17 × 10-5M⊙ yr-1 in 2014. We investigate possible scenarios that could have generated the complex circumstellar environment revealed by our multiwavelength data.es_CL
dc.description.urihttps://academic.oup.com/mnras/article-lookup/doi/10.1093/mnras/stw3074
dc.language.isoenes_CL
dc.publisherOXFORD UNIV PRESSes_CL
dc.subjectCircumstellar matteres_CL
dc.subjectInfrared: starses_CL
dc.subjectOutflowses_CL
dc.subjectRadio continuum: starses_CL
dc.subjectStars: early-typees_CL
dc.subjectStars: individual: HR Cares_CL
dc.subjectStars: windses_CL
dc.titleExploring the multifaceted circumstellar environment of the luminous blue variable HR Carinaees_CL
dc.typeArticlees_CL


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