The sudden appearance of CO emission in LHA 115-S 65
- Autores
- Oksala, M. E.; Kraus, M.; Arias, María Laura; Borges Fernandes, M.; Cidale, Lydia Sonia; Muratore, María Florencia; Curé, M.
- Año de publicación
- 2012
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- Molecular emission has been detected in several Magellanic Cloud B[e] supergiants. In this Letter, we report on the detection of CO band head emission in the B[e] supergiant LHA 115-S 65, and present a K-band near-infrared spectrum obtained with the Spectrograph for INtegral Field Observation in the Near-Infrared (SINFONI; R = 4500) on the ESO VLT UT4 telescope. The observed molecular band head emission in S65 is quite surprising in the light of a previous non-detection by McGregor, Hyland & McGinn, as well as a high-resolution (R = 50 000) Gemini/Phoenix spectrum of this star taken nine months earlier showing no emission. Based on analysis of the optical spectrum by Kraus, Borges Fernandes & de Aráujo, we suspect that the sudden appearance of molecular emission could be due to density buildup in an outflowing viscous disc, as seen for Be stars. This new discovery, combined with variability in two other similar evolved massive stars, indicates an evolutionary link between B[e] supergiants and luminous blue variables.
Facultad de Ciencias Astronómicas y Geofísicas - Materia
-
Ciencias Astronómicas
Be
Circumstellar matter
Outflows
Stars: emission-line
Stars: individual: LHA115-S 65
Stars: winds
Supergiants - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- http://creativecommons.org/licenses/by-nc-sa/4.0/
- Repositorio
- Institución
- Universidad Nacional de La Plata
- OAI Identificador
- oai:sedici.unlp.edu.ar:10915/84628
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The sudden appearance of CO emission in LHA 115-S 65Oksala, M. E.Kraus, M.Arias, María LauraBorges Fernandes, M.Cidale, Lydia SoniaMuratore, María FlorenciaCuré, M.Ciencias AstronómicasBeCircumstellar matterOutflowsStars: emission-lineStars: individual: LHA115-S 65Stars: windsSupergiantsMolecular emission has been detected in several Magellanic Cloud B[e] supergiants. In this Letter, we report on the detection of CO band head emission in the B[e] supergiant LHA 115-S 65, and present a K-band near-infrared spectrum obtained with the Spectrograph for INtegral Field Observation in the Near-Infrared (SINFONI; R = 4500) on the ESO VLT UT4 telescope. The observed molecular band head emission in S65 is quite surprising in the light of a previous non-detection by McGregor, Hyland & McGinn, as well as a high-resolution (R = 50 000) Gemini/Phoenix spectrum of this star taken nine months earlier showing no emission. Based on analysis of the optical spectrum by Kraus, Borges Fernandes & de Aráujo, we suspect that the sudden appearance of molecular emission could be due to density buildup in an outflowing viscous disc, as seen for Be stars. This new discovery, combined with variability in two other similar evolved massive stars, indicates an evolutionary link between B[e] supergiants and luminous blue variables.Facultad de Ciencias Astronómicas y Geofísicas2012-10-01info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfL56-L60http://sedici.unlp.edu.ar/handle/10915/84628enginfo:eu-repo/semantics/altIdentifier/issn/1745-3925info:eu-repo/semantics/altIdentifier/doi/10.1111/j.1745-3933.2012.01323.xinfo:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by-nc-sa/4.0/Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-09-29T11:16:01Zoai:sedici.unlp.edu.ar:10915/84628Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-09-29 11:16:01.51SEDICI (UNLP) - Universidad Nacional de La Platafalse |
dc.title.none.fl_str_mv |
The sudden appearance of CO emission in LHA 115-S 65 |
title |
The sudden appearance of CO emission in LHA 115-S 65 |
spellingShingle |
The sudden appearance of CO emission in LHA 115-S 65 Oksala, M. E. Ciencias Astronómicas Be Circumstellar matter Outflows Stars: emission-line Stars: individual: LHA115-S 65 Stars: winds Supergiants |
title_short |
The sudden appearance of CO emission in LHA 115-S 65 |
title_full |
The sudden appearance of CO emission in LHA 115-S 65 |
title_fullStr |
The sudden appearance of CO emission in LHA 115-S 65 |
title_full_unstemmed |
The sudden appearance of CO emission in LHA 115-S 65 |
title_sort |
The sudden appearance of CO emission in LHA 115-S 65 |
dc.creator.none.fl_str_mv |
Oksala, M. E. Kraus, M. Arias, María Laura Borges Fernandes, M. Cidale, Lydia Sonia Muratore, María Florencia Curé, M. |
author |
Oksala, M. E. |
author_facet |
Oksala, M. E. Kraus, M. Arias, María Laura Borges Fernandes, M. Cidale, Lydia Sonia Muratore, María Florencia Curé, M. |
author_role |
author |
author2 |
Kraus, M. Arias, María Laura Borges Fernandes, M. Cidale, Lydia Sonia Muratore, María Florencia Curé, M. |
author2_role |
author author author author author author |
dc.subject.none.fl_str_mv |
Ciencias Astronómicas Be Circumstellar matter Outflows Stars: emission-line Stars: individual: LHA115-S 65 Stars: winds Supergiants |
topic |
Ciencias Astronómicas Be Circumstellar matter Outflows Stars: emission-line Stars: individual: LHA115-S 65 Stars: winds Supergiants |
dc.description.none.fl_txt_mv |
Molecular emission has been detected in several Magellanic Cloud B[e] supergiants. In this Letter, we report on the detection of CO band head emission in the B[e] supergiant LHA 115-S 65, and present a K-band near-infrared spectrum obtained with the Spectrograph for INtegral Field Observation in the Near-Infrared (SINFONI; R = 4500) on the ESO VLT UT4 telescope. The observed molecular band head emission in S65 is quite surprising in the light of a previous non-detection by McGregor, Hyland & McGinn, as well as a high-resolution (R = 50 000) Gemini/Phoenix spectrum of this star taken nine months earlier showing no emission. Based on analysis of the optical spectrum by Kraus, Borges Fernandes & de Aráujo, we suspect that the sudden appearance of molecular emission could be due to density buildup in an outflowing viscous disc, as seen for Be stars. This new discovery, combined with variability in two other similar evolved massive stars, indicates an evolutionary link between B[e] supergiants and luminous blue variables. Facultad de Ciencias Astronómicas y Geofísicas |
description |
Molecular emission has been detected in several Magellanic Cloud B[e] supergiants. In this Letter, we report on the detection of CO band head emission in the B[e] supergiant LHA 115-S 65, and present a K-band near-infrared spectrum obtained with the Spectrograph for INtegral Field Observation in the Near-Infrared (SINFONI; R = 4500) on the ESO VLT UT4 telescope. The observed molecular band head emission in S65 is quite surprising in the light of a previous non-detection by McGregor, Hyland & McGinn, as well as a high-resolution (R = 50 000) Gemini/Phoenix spectrum of this star taken nine months earlier showing no emission. Based on analysis of the optical spectrum by Kraus, Borges Fernandes & de Aráujo, we suspect that the sudden appearance of molecular emission could be due to density buildup in an outflowing viscous disc, as seen for Be stars. This new discovery, combined with variability in two other similar evolved massive stars, indicates an evolutionary link between B[e] supergiants and luminous blue variables. |
publishDate |
2012 |
dc.date.none.fl_str_mv |
2012-10-01 |
dc.type.none.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion Articulo 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://sedici.unlp.edu.ar/handle/10915/84628 |
url |
http://sedici.unlp.edu.ar/handle/10915/84628 |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/issn/1745-3925 info:eu-repo/semantics/altIdentifier/doi/10.1111/j.1745-3933.2012.01323.x |
dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) |
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openAccess |
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http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) |
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application/pdf L56-L60 |
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