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
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/43227
Ver los metadatos del registro completo
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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 Técnicas2025-09-29T09:57:33Zoai: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:34982025-09-29 09:57:34.138CONICET 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 |
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1844613721362530304 |
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13.070432 |