Simultaneous k- and l-band spectroscopy of be stars: Circumstellar envelope properties from hydrogen emission lines
- Autores
- Granada, Anahí; Arias, María Laura; Cidale, Lydia Sonia
- Año de publicación
- 2010
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- We present medium-resolution K- and L-band spectra of a sample of eight Be stars, obtained with Gemini/NIRI. The IR K and L bands contain many lines of different hydrogen series that are used as a diagnosis to the physical conditions in the circumstellar environments. We make an analysis on the optical depths of the line-forming regions based on the intensity ratios of Pfγ and Brα lines, the behavior of Humphreys' series, and the fluxes of Brα and Brγ lines. All our targets show spectroscopic and photometric long-term variability; thus, time-resolved K- and L-band spectroscopy is an ideal tool for studying the structure and evolution of the innermost regions of the envelope and to test models on the disk-forming mechanism. We note that the instrumental configuration used allowed us to obtain good quality IR observations and to take profit of Gemini band 3 observing time (allocation time for ranked programs in which the observing conditions are relaxed).
Facultad de Ciencias Astronómicas y Geofísicas
Instituto de Astrofísica de La Plata (CONICET- Universidad Nacional de La Plata) - Materia
-
Ciencias Astronómicas
Circumstellar matter
Formation
Stars: activity
Techniques: spectroscopic - 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:10915/82472
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Simultaneous k- and l-band spectroscopy of be stars: Circumstellar envelope properties from hydrogen emission linesGranada, AnahíArias, María LauraCidale, Lydia SoniaCiencias AstronómicasCircumstellar matterFormationStars: activityTechniques: spectroscopicWe present medium-resolution K- and L-band spectra of a sample of eight Be stars, obtained with Gemini/NIRI. The IR K and L bands contain many lines of different hydrogen series that are used as a diagnosis to the physical conditions in the circumstellar environments. We make an analysis on the optical depths of the line-forming regions based on the intensity ratios of Pfγ and Brα lines, the behavior of Humphreys' series, and the fluxes of Brα and Brγ lines. All our targets show spectroscopic and photometric long-term variability; thus, time-resolved K- and L-band spectroscopy is an ideal tool for studying the structure and evolution of the innermost regions of the envelope and to test models on the disk-forming mechanism. We note that the instrumental configuration used allowed us to obtain good quality IR observations and to take profit of Gemini band 3 observing time (allocation time for ranked programs in which the observing conditions are relaxed).Facultad de Ciencias Astronómicas y GeofísicasInstituto de Astrofísica de La Plata (CONICET- Universidad Nacional de La Plata)2010-04-08info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdf1983-1992http://sedici.unlp.edu.ar/handle/10915/82472enginfo:eu-repo/semantics/altIdentifier/issn/00046256info:eu-repo/semantics/altIdentifier/doi/10.1088/0004-6256/139/5/1983info: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:UNLP2025-09-29T11:15:31Zoai:sedici.unlp.edu.ar:10915/82472Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-09-29 11:15:31.356SEDICI (UNLP) - Universidad Nacional de La Platafalse |
dc.title.none.fl_str_mv |
Simultaneous k- and l-band spectroscopy of be stars: Circumstellar envelope properties from hydrogen emission lines |
title |
Simultaneous k- and l-band spectroscopy of be stars: Circumstellar envelope properties from hydrogen emission lines |
spellingShingle |
Simultaneous k- and l-band spectroscopy of be stars: Circumstellar envelope properties from hydrogen emission lines Granada, Anahí Ciencias Astronómicas Circumstellar matter Formation Stars: activity Techniques: spectroscopic |
title_short |
Simultaneous k- and l-band spectroscopy of be stars: Circumstellar envelope properties from hydrogen emission lines |
title_full |
Simultaneous k- and l-band spectroscopy of be stars: Circumstellar envelope properties from hydrogen emission lines |
title_fullStr |
Simultaneous k- and l-band spectroscopy of be stars: Circumstellar envelope properties from hydrogen emission lines |
title_full_unstemmed |
Simultaneous k- and l-band spectroscopy of be stars: Circumstellar envelope properties from hydrogen emission lines |
title_sort |
Simultaneous k- and l-band spectroscopy of be stars: Circumstellar envelope properties from hydrogen emission lines |
dc.creator.none.fl_str_mv |
Granada, Anahí Arias, María Laura Cidale, Lydia Sonia |
author |
Granada, Anahí |
author_facet |
Granada, Anahí Arias, María Laura Cidale, Lydia Sonia |
author_role |
author |
author2 |
Arias, María Laura Cidale, Lydia Sonia |
author2_role |
author author |
dc.subject.none.fl_str_mv |
Ciencias Astronómicas Circumstellar matter Formation Stars: activity Techniques: spectroscopic |
topic |
Ciencias Astronómicas Circumstellar matter Formation Stars: activity Techniques: spectroscopic |
dc.description.none.fl_txt_mv |
We present medium-resolution K- and L-band spectra of a sample of eight Be stars, obtained with Gemini/NIRI. The IR K and L bands contain many lines of different hydrogen series that are used as a diagnosis to the physical conditions in the circumstellar environments. We make an analysis on the optical depths of the line-forming regions based on the intensity ratios of Pfγ and Brα lines, the behavior of Humphreys' series, and the fluxes of Brα and Brγ lines. All our targets show spectroscopic and photometric long-term variability; thus, time-resolved K- and L-band spectroscopy is an ideal tool for studying the structure and evolution of the innermost regions of the envelope and to test models on the disk-forming mechanism. We note that the instrumental configuration used allowed us to obtain good quality IR observations and to take profit of Gemini band 3 observing time (allocation time for ranked programs in which the observing conditions are relaxed). Facultad de Ciencias Astronómicas y Geofísicas Instituto de Astrofísica de La Plata (CONICET- Universidad Nacional de La Plata) |
description |
We present medium-resolution K- and L-band spectra of a sample of eight Be stars, obtained with Gemini/NIRI. The IR K and L bands contain many lines of different hydrogen series that are used as a diagnosis to the physical conditions in the circumstellar environments. We make an analysis on the optical depths of the line-forming regions based on the intensity ratios of Pfγ and Brα lines, the behavior of Humphreys' series, and the fluxes of Brα and Brγ lines. All our targets show spectroscopic and photometric long-term variability; thus, time-resolved K- and L-band spectroscopy is an ideal tool for studying the structure and evolution of the innermost regions of the envelope and to test models on the disk-forming mechanism. We note that the instrumental configuration used allowed us to obtain good quality IR observations and to take profit of Gemini band 3 observing time (allocation time for ranked programs in which the observing conditions are relaxed). |
publishDate |
2010 |
dc.date.none.fl_str_mv |
2010-04-08 |
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/10915/82472 |
url |
http://sedici.unlp.edu.ar/handle/10915/82472 |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/issn/00046256 info:eu-repo/semantics/altIdentifier/doi/10.1088/0004-6256/139/5/1983 |
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) |
eu_rights_str_mv |
openAccess |
rights_invalid_str_mv |
http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) |
dc.format.none.fl_str_mv |
application/pdf 1983-1992 |
dc.source.none.fl_str_mv |
reponame:SEDICI (UNLP) instname:Universidad Nacional de La Plata instacron:UNLP |
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SEDICI (UNLP) |
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Universidad Nacional de La Plata |
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SEDICI (UNLP) - Universidad Nacional de La Plata |
repository.mail.fl_str_mv |
alira@sedici.unlp.edu.ar |
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