Analysis of the Si II and Si III DR Processes Applied to Stellar Envelopes
- Autores
- Cruzado, Alicia; Ringuelet, Adela Emilia; Di Rocco, Héctor Oscar
- Año de publicación
- 2001
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- In an earlier attempt to explain the observed excess in the IR flux of Be stars, we have analyzed the dielectronic recombination (DR) of Mg II in stellar envelopes and the influence of this atomic process on the stellar flux. In the present paper, we study the DR of other ions with astrophysical significance, namely, Si II and Si III, and reach the conclusion that Si II may also contribute to the IR excess in Be stars.
Facultad de Ciencias Astronómicas y Geofísicas - Materia
-
Ciencias Astronómicas
Geofísica, astronomía y astrofísica
atomic processes
infrared: stars - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- http://creativecommons.org/licenses/by-nc-nd/4.0/
- Repositorio
- Institución
- Universidad Nacional de La Plata
- OAI Identificador
- oai:sedici.unlp.edu.ar:10915/2083
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Analysis of the Si II and Si III DR Processes Applied to Stellar EnvelopesCruzado, AliciaRinguelet, Adela EmiliaDi Rocco, Héctor OscarCiencias AstronómicasGeofísica, astronomía y astrofísicaatomic processesinfrared: starsIn an earlier attempt to explain the observed excess in the IR flux of Be stars, we have analyzed the dielectronic recombination (DR) of Mg II in stellar envelopes and the influence of this atomic process on the stellar flux. In the present paper, we study the DR of other ions with astrophysical significance, namely, Si II and Si III, and reach the conclusion that Si II may also contribute to the IR excess in Be stars.Facultad de Ciencias Astronómicas y Geofísicas2001info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdf571-577http://sedici.unlp.edu.ar/handle/10915/2083enginfo:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.1086/321375/fulltext/info:eu-repo/semantics/altIdentifier/issn/0004-637Xinfo:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by-nc-nd/4.0/Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International (CC BY-NC-ND 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-09-03T10:21:37Zoai:sedici.unlp.edu.ar:10915/2083Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-09-03 10:21:38.176SEDICI (UNLP) - Universidad Nacional de La Platafalse |
dc.title.none.fl_str_mv |
Analysis of the Si II and Si III DR Processes Applied to Stellar Envelopes |
title |
Analysis of the Si II and Si III DR Processes Applied to Stellar Envelopes |
spellingShingle |
Analysis of the Si II and Si III DR Processes Applied to Stellar Envelopes Cruzado, Alicia Ciencias Astronómicas Geofísica, astronomía y astrofísica atomic processes infrared: stars |
title_short |
Analysis of the Si II and Si III DR Processes Applied to Stellar Envelopes |
title_full |
Analysis of the Si II and Si III DR Processes Applied to Stellar Envelopes |
title_fullStr |
Analysis of the Si II and Si III DR Processes Applied to Stellar Envelopes |
title_full_unstemmed |
Analysis of the Si II and Si III DR Processes Applied to Stellar Envelopes |
title_sort |
Analysis of the Si II and Si III DR Processes Applied to Stellar Envelopes |
dc.creator.none.fl_str_mv |
Cruzado, Alicia Ringuelet, Adela Emilia Di Rocco, Héctor Oscar |
author |
Cruzado, Alicia |
author_facet |
Cruzado, Alicia Ringuelet, Adela Emilia Di Rocco, Héctor Oscar |
author_role |
author |
author2 |
Ringuelet, Adela Emilia Di Rocco, Héctor Oscar |
author2_role |
author author |
dc.subject.none.fl_str_mv |
Ciencias Astronómicas Geofísica, astronomía y astrofísica atomic processes infrared: stars |
topic |
Ciencias Astronómicas Geofísica, astronomía y astrofísica atomic processes infrared: stars |
dc.description.none.fl_txt_mv |
In an earlier attempt to explain the observed excess in the IR flux of Be stars, we have analyzed the dielectronic recombination (DR) of Mg II in stellar envelopes and the influence of this atomic process on the stellar flux. In the present paper, we study the DR of other ions with astrophysical significance, namely, Si II and Si III, and reach the conclusion that Si II may also contribute to the IR excess in Be stars. Facultad de Ciencias Astronómicas y Geofísicas |
description |
In an earlier attempt to explain the observed excess in the IR flux of Be stars, we have analyzed the dielectronic recombination (DR) of Mg II in stellar envelopes and the influence of this atomic process on the stellar flux. In the present paper, we study the DR of other ions with astrophysical significance, namely, Si II and Si III, and reach the conclusion that Si II may also contribute to the IR excess in Be stars. |
publishDate |
2001 |
dc.date.none.fl_str_mv |
2001 |
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/10915/2083 |
url |
http://sedici.unlp.edu.ar/handle/10915/2083 |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.1086/321375/fulltext/ info:eu-repo/semantics/altIdentifier/issn/0004-637X |
dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by-nc-nd/4.0/ Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International (CC BY-NC-ND 4.0) |
eu_rights_str_mv |
openAccess |
rights_invalid_str_mv |
http://creativecommons.org/licenses/by-nc-nd/4.0/ Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International (CC BY-NC-ND 4.0) |
dc.format.none.fl_str_mv |
application/pdf 571-577 |
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