A three-decade outburst of the LMC luminous blue variable R127 draws to a close

Autores
Walborn, Nolan Revere; Stahl, O.; Gamen, Roberto Claudio; Szeifert, T.; Morrell, Nidia Irene; Smith, N. I.; Howarth, I. D.; Humphreys, R. M.; Bond, H. E.; Lennon, D. J.
Año de publicación
2008
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
The paradigmatic luminous blue variable R127 in the Large Magellanic Cloud has been found in the intermediate, peculiar early-B state, and substantially fainter in visual light, signaling the final decline from its major outburst that began between 1978 and 1980. This transformation was detected in 2008 January, but archival data show that it began between early 2005 and early 2007. In fact, significant changes from the maximum, peculiar A-type spectrum, which was maintained from 1986 through 1998, had already begun the following year, coinciding with a steep drop in visual light. We show detailed correspondences between the spectrum and light, in which the decline mimics the rise. Moreover, these trends are not monotonic but are characterized by multiple spikes and dips, which may provide constraints on the unknown outburst mechanism. Intensive photometric and spectroscopic monitoring of R127 should now resume, to follow the decline presumably back to the quiescent Ofpe/WN9 state, in order to fully document the remainder of this unique observational opportunity.
Fil: Walborn, Nolan Revere. Space Telescope Science Institute; Estados Unidos
Fil: Stahl, O.. Zentrum für Astronomie der Universität Heidelberg; Alemania
Fil: Gamen, Roberto Claudio. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan. Complejo Astronómico ; Argentina
Fil: Szeifert, T.. European Southern Observatory; Chile
Fil: Morrell, Nidia Irene. Las Campanas Observatory; Chile
Fil: Smith, N. I.. University of California; Estados Unidos
Fil: Howarth, I. D.. University College London; Reino Unido
Fil: Humphreys, R. M.. University of Minnesota; Estados Unidos
Fil: Bond, H. E.. Space Telescope Science Institute; Estados Unidos
Fil: Lennon, D. J.. Space Telescope Science Institute; Estados Unidos
Materia
Magellanic Clouds
Early type stars
R127
HDE 269858
Variable stars
Winds
Outflows
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/43227
Acceder
id CONICETDig_2006bf71afabaedb2e2e8385f4b51457
oai_identifier_str oai:ri.conicet.gov.ar:11336/43227
network_acronym_str CONICETDig
repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling A three-decade outburst of the LMC luminous blue variable R127 draws to a closeWalborn, Nolan RevereStahl, O.Gamen, Roberto ClaudioSzeifert, T.Morrell, Nidia IreneSmith, N. I.Howarth, I. D.Humphreys, R. M.Bond, H. E.Lennon, D. J.Magellanic CloudsEarly type starsR127HDE 269858Variable starsWindsOutflowshttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1The paradigmatic luminous blue variable R127 in the Large Magellanic Cloud has been found in the intermediate, peculiar early-B state, and substantially fainter in visual light, signaling the final decline from its major outburst that began between 1978 and 1980. This transformation was detected in 2008 January, but archival data show that it began between early 2005 and early 2007. In fact, significant changes from the maximum, peculiar A-type spectrum, which was maintained from 1986 through 1998, had already begun the following year, coinciding with a steep drop in visual light. We show detailed correspondences between the spectrum and light, in which the decline mimics the rise. Moreover, these trends are not monotonic but are characterized by multiple spikes and dips, which may provide constraints on the unknown outburst mechanism. Intensive photometric and spectroscopic monitoring of R127 should now resume, to follow the decline presumably back to the quiescent Ofpe/WN9 state, in order to fully document the remainder of this unique observational opportunity.Fil: Walborn, Nolan Revere. Space Telescope Science Institute; Estados UnidosFil: Stahl, O.. Zentrum für Astronomie der Universität Heidelberg; AlemaniaFil: Gamen, Roberto Claudio. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan. Complejo Astronómico ; ArgentinaFil: Szeifert, T.. European Southern Observatory; ChileFil: Morrell, Nidia Irene. Las Campanas Observatory; ChileFil: Smith, N. I.. University of California; Estados UnidosFil: Howarth, I. D.. University College London; Reino UnidoFil: Humphreys, R. M.. University of Minnesota; Estados UnidosFil: Bond, H. E.. Space Telescope Science Institute; Estados UnidosFil: Lennon, D. J.. Space Telescope Science Institute; Estados UnidosIOP Publishing2008-12info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/43227Walborn, Nolan Revere; Stahl, O.; Gamen, Roberto Claudio; Szeifert, T.; Morrell, Nidia Irene; et al.; A three-decade outburst of the LMC luminous blue variable R127 draws to a close; IOP Publishing; Astrophysical Journal; 683; 12-2008; L33-L360004-637XCONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1086/591525info:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.1086/591525/metainfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-15T14:52:55Zoai:ri.conicet.gov.ar:11336/43227instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-10-15 14:52:55.942CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv A three-decade outburst of the LMC luminous blue variable R127 draws to a close
title A three-decade outburst of the LMC luminous blue variable R127 draws to a close
spellingShingle A three-decade outburst of the LMC luminous blue variable R127 draws to a close
Walborn, Nolan Revere
Magellanic Clouds
Early type stars
R127
HDE 269858
Variable stars
Winds
Outflows
title_short A three-decade outburst of the LMC luminous blue variable R127 draws to a close
title_full A three-decade outburst of the LMC luminous blue variable R127 draws to a close
title_fullStr A three-decade outburst of the LMC luminous blue variable R127 draws to a close
title_full_unstemmed A three-decade outburst of the LMC luminous blue variable R127 draws to a close
title_sort A three-decade outburst of the LMC luminous blue variable R127 draws to a close
dc.creator.none.fl_str_mv Walborn, Nolan Revere
Stahl, O.
Gamen, Roberto Claudio
Szeifert, T.
Morrell, Nidia Irene
Smith, N. I.
Howarth, I. D.
Humphreys, R. M.
Bond, H. E.
Lennon, D. J.
author Walborn, Nolan Revere
author_facet Walborn, Nolan Revere
Stahl, O.
Gamen, Roberto Claudio
Szeifert, T.
Morrell, Nidia Irene
Smith, N. I.
Howarth, I. D.
Humphreys, R. M.
Bond, H. E.
Lennon, D. J.
author_role author
author2 Stahl, O.
Gamen, Roberto Claudio
Szeifert, T.
Morrell, Nidia Irene
Smith, N. I.
Howarth, I. D.
Humphreys, R. M.
Bond, H. E.
Lennon, D. J.
author2_role author
author
author
author
author
author
author
author
author
dc.subject.none.fl_str_mv Magellanic Clouds
Early type stars
R127
HDE 269858
Variable stars
Winds
Outflows
topic Magellanic Clouds
Early type stars
R127
HDE 269858
Variable stars
Winds
Outflows
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv The paradigmatic luminous blue variable R127 in the Large Magellanic Cloud has been found in the intermediate, peculiar early-B state, and substantially fainter in visual light, signaling the final decline from its major outburst that began between 1978 and 1980. This transformation was detected in 2008 January, but archival data show that it began between early 2005 and early 2007. In fact, significant changes from the maximum, peculiar A-type spectrum, which was maintained from 1986 through 1998, had already begun the following year, coinciding with a steep drop in visual light. We show detailed correspondences between the spectrum and light, in which the decline mimics the rise. Moreover, these trends are not monotonic but are characterized by multiple spikes and dips, which may provide constraints on the unknown outburst mechanism. Intensive photometric and spectroscopic monitoring of R127 should now resume, to follow the decline presumably back to the quiescent Ofpe/WN9 state, in order to fully document the remainder of this unique observational opportunity.
Fil: Walborn, Nolan Revere. Space Telescope Science Institute; Estados Unidos
Fil: Stahl, O.. Zentrum für Astronomie der Universität Heidelberg; Alemania
Fil: Gamen, Roberto Claudio. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan. Complejo Astronómico ; Argentina
Fil: Szeifert, T.. European Southern Observatory; Chile
Fil: Morrell, Nidia Irene. Las Campanas Observatory; Chile
Fil: Smith, N. I.. University of California; Estados Unidos
Fil: Howarth, I. D.. University College London; Reino Unido
Fil: Humphreys, R. M.. University of Minnesota; Estados Unidos
Fil: Bond, H. E.. Space Telescope Science Institute; Estados Unidos
Fil: Lennon, D. J.. Space Telescope Science Institute; Estados Unidos
description The paradigmatic luminous blue variable R127 in the Large Magellanic Cloud has been found in the intermediate, peculiar early-B state, and substantially fainter in visual light, signaling the final decline from its major outburst that began between 1978 and 1980. This transformation was detected in 2008 January, but archival data show that it began between early 2005 and early 2007. In fact, significant changes from the maximum, peculiar A-type spectrum, which was maintained from 1986 through 1998, had already begun the following year, coinciding with a steep drop in visual light. We show detailed correspondences between the spectrum and light, in which the decline mimics the rise. Moreover, these trends are not monotonic but are characterized by multiple spikes and dips, which may provide constraints on the unknown outburst mechanism. Intensive photometric and spectroscopic monitoring of R127 should now resume, to follow the decline presumably back to the quiescent Ofpe/WN9 state, in order to fully document the remainder of this unique observational opportunity.
publishDate 2008
dc.date.none.fl_str_mv 2008-12
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
http://purl.org/coar/resource_type/c_6501
info:ar-repo/semantics/articulo
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://hdl.handle.net/11336/43227
Walborn, Nolan Revere; Stahl, O.; Gamen, Roberto Claudio; Szeifert, T.; Morrell, Nidia Irene; et al.; A three-decade outburst of the LMC luminous blue variable R127 draws to a close; IOP Publishing; Astrophysical Journal; 683; 12-2008; L33-L36
0004-637X
CONICET Digital
CONICET
url http://hdl.handle.net/11336/43227
identifier_str_mv Walborn, Nolan Revere; Stahl, O.; Gamen, Roberto Claudio; Szeifert, T.; Morrell, Nidia Irene; et al.; A three-decade outburst of the LMC luminous blue variable R127 draws to a close; IOP Publishing; Astrophysical Journal; 683; 12-2008; L33-L36
0004-637X
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/doi/10.1086/591525
info:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.1086/591525/meta
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.format.none.fl_str_mv application/pdf
application/pdf
dc.publisher.none.fl_str_mv IOP Publishing
publisher.none.fl_str_mv IOP Publishing
dc.source.none.fl_str_mv reponame:CONICET Digital (CONICET)
instname:Consejo Nacional de Investigaciones Científicas y Técnicas
reponame_str CONICET Digital (CONICET)
collection CONICET Digital (CONICET)
instname_str Consejo Nacional de Investigaciones Científicas y Técnicas
repository.name.fl_str_mv CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas
repository.mail.fl_str_mv dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar
_version_ 1846083058621480960
score 13.22299

Publicaciones similares