Detection of variable Si II, Mn II, and Fe II emission lines in the magnetic Bp star a Centauri
- Autores
- Hubrig, S.; Gonzalez, Jorge Federico
- Año de publicación
- 2007
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- Context. The nature of non-variable high-excitation emission lines detected in the optical spectra of normal late-B type and chemically peculiar HgMn and PGa stars is still poorly understood. Aims. To better understand the origin of the weak emission lines in B type stars it is especially important to investigate the spectra of a variety of stars to search for correlations between the emergence of these lines and fundamental stellar parameters. Methods. We have acquired high resolution UVES spectra for the sharp-lined magnetic helium-variable star a Cen over the rotation period of 8.82 d to search for the presence of weak emission lines. Results. For the first time we present observational evidence for the appearance of variable high-excitation Si II, Mn II and Fe II emission lines in a magnetic Bp star. Si II emissions are the strongest at the phase corresponding to the maximum strength of He I lines. Mn II and Fe II emissions vary in antiphase to the He I lines. A correlation is found between the probable location of Mn and Fe surface spots and the strength of the emission lines. On the basis of the currently available data it seems possible that the same kind of selective excitation process is working in the atmospheres of objects within a broad parameter space which could be defined by age, effective temperature, chemical composition, rotational velocity, and magnetic field. Neutral iron lines previously reported to appear broad and shallow at certain phases are not detected in our spectra, although two of them are identified as He I forbidden lines, snowing maximum strength at the phase of the passage of the He rich region across the visible disk.
Fil: Hubrig, S.. European Southern Observatory Santiago; Chile
Fil: Gonzalez, Jorge Federico. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan. Complejo Astronómico "El Leoncito". Universidad Nacional de Córdoba. Complejo Astronómico "El Leoncito". Universidad Nacional de la Plata. Complejo Astronómico "El Leoncito". Universidad Nacional de San Juan. Complejo Astronómico "El Leoncito"; Argentina - Materia
-
LINE: IDENTIFICATION
STARS: ABUNDANCES
STARS: CHEMICALLY PECULIAR
STARS: EMISSION-LINE, BE
STARS: INDIVIDUAL: HD 125823 - 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:11336/213844
Ver los metadatos del registro completo
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oai:ri.conicet.gov.ar:11336/213844 |
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3498 |
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CONICET Digital (CONICET) |
spelling |
Detection of variable Si II, Mn II, and Fe II emission lines in the magnetic Bp star a CentauriHubrig, S.Gonzalez, Jorge FedericoLINE: IDENTIFICATIONSTARS: ABUNDANCESSTARS: CHEMICALLY PECULIARSTARS: EMISSION-LINE, BESTARS: INDIVIDUAL: HD 125823https://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Context. The nature of non-variable high-excitation emission lines detected in the optical spectra of normal late-B type and chemically peculiar HgMn and PGa stars is still poorly understood. Aims. To better understand the origin of the weak emission lines in B type stars it is especially important to investigate the spectra of a variety of stars to search for correlations between the emergence of these lines and fundamental stellar parameters. Methods. We have acquired high resolution UVES spectra for the sharp-lined magnetic helium-variable star a Cen over the rotation period of 8.82 d to search for the presence of weak emission lines. Results. For the first time we present observational evidence for the appearance of variable high-excitation Si II, Mn II and Fe II emission lines in a magnetic Bp star. Si II emissions are the strongest at the phase corresponding to the maximum strength of He I lines. Mn II and Fe II emissions vary in antiphase to the He I lines. A correlation is found between the probable location of Mn and Fe surface spots and the strength of the emission lines. On the basis of the currently available data it seems possible that the same kind of selective excitation process is working in the atmospheres of objects within a broad parameter space which could be defined by age, effective temperature, chemical composition, rotational velocity, and magnetic field. Neutral iron lines previously reported to appear broad and shallow at certain phases are not detected in our spectra, although two of them are identified as He I forbidden lines, snowing maximum strength at the phase of the passage of the He rich region across the visible disk.Fil: Hubrig, S.. European Southern Observatory Santiago; ChileFil: Gonzalez, Jorge Federico. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan. Complejo Astronómico "El Leoncito". Universidad Nacional de Córdoba. Complejo Astronómico "El Leoncito". Universidad Nacional de la Plata. Complejo Astronómico "El Leoncito". Universidad Nacional de San Juan. Complejo Astronómico "El Leoncito"; ArgentinaEDP Sciences2007-12info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/213844Hubrig, S.; Gonzalez, Jorge Federico; Detection of variable Si II, Mn II, and Fe II emission lines in the magnetic Bp star a Centauri; EDP Sciences; Astronomy and Astrophysics; 466; 3; 12-2007; 1083-10870004-6361CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361:20066738info:eu-repo/semantics/altIdentifier/url/https://www.aanda.org/articles/aa/abs/2007/18/aa6738-06/aa6738-06.htmlinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:42:54Zoai:ri.conicet.gov.ar:11336/213844instacron: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 09:42:54.643CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
Detection of variable Si II, Mn II, and Fe II emission lines in the magnetic Bp star a Centauri |
title |
Detection of variable Si II, Mn II, and Fe II emission lines in the magnetic Bp star a Centauri |
spellingShingle |
Detection of variable Si II, Mn II, and Fe II emission lines in the magnetic Bp star a Centauri Hubrig, S. LINE: IDENTIFICATION STARS: ABUNDANCES STARS: CHEMICALLY PECULIAR STARS: EMISSION-LINE, BE STARS: INDIVIDUAL: HD 125823 |
title_short |
Detection of variable Si II, Mn II, and Fe II emission lines in the magnetic Bp star a Centauri |
title_full |
Detection of variable Si II, Mn II, and Fe II emission lines in the magnetic Bp star a Centauri |
title_fullStr |
Detection of variable Si II, Mn II, and Fe II emission lines in the magnetic Bp star a Centauri |
title_full_unstemmed |
Detection of variable Si II, Mn II, and Fe II emission lines in the magnetic Bp star a Centauri |
title_sort |
Detection of variable Si II, Mn II, and Fe II emission lines in the magnetic Bp star a Centauri |
dc.creator.none.fl_str_mv |
Hubrig, S. Gonzalez, Jorge Federico |
author |
Hubrig, S. |
author_facet |
Hubrig, S. Gonzalez, Jorge Federico |
author_role |
author |
author2 |
Gonzalez, Jorge Federico |
author2_role |
author |
dc.subject.none.fl_str_mv |
LINE: IDENTIFICATION STARS: ABUNDANCES STARS: CHEMICALLY PECULIAR STARS: EMISSION-LINE, BE STARS: INDIVIDUAL: HD 125823 |
topic |
LINE: IDENTIFICATION STARS: ABUNDANCES STARS: CHEMICALLY PECULIAR STARS: EMISSION-LINE, BE STARS: INDIVIDUAL: HD 125823 |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
Context. The nature of non-variable high-excitation emission lines detected in the optical spectra of normal late-B type and chemically peculiar HgMn and PGa stars is still poorly understood. Aims. To better understand the origin of the weak emission lines in B type stars it is especially important to investigate the spectra of a variety of stars to search for correlations between the emergence of these lines and fundamental stellar parameters. Methods. We have acquired high resolution UVES spectra for the sharp-lined magnetic helium-variable star a Cen over the rotation period of 8.82 d to search for the presence of weak emission lines. Results. For the first time we present observational evidence for the appearance of variable high-excitation Si II, Mn II and Fe II emission lines in a magnetic Bp star. Si II emissions are the strongest at the phase corresponding to the maximum strength of He I lines. Mn II and Fe II emissions vary in antiphase to the He I lines. A correlation is found between the probable location of Mn and Fe surface spots and the strength of the emission lines. On the basis of the currently available data it seems possible that the same kind of selective excitation process is working in the atmospheres of objects within a broad parameter space which could be defined by age, effective temperature, chemical composition, rotational velocity, and magnetic field. Neutral iron lines previously reported to appear broad and shallow at certain phases are not detected in our spectra, although two of them are identified as He I forbidden lines, snowing maximum strength at the phase of the passage of the He rich region across the visible disk. Fil: Hubrig, S.. European Southern Observatory Santiago; Chile Fil: Gonzalez, Jorge Federico. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan. Complejo Astronómico "El Leoncito". Universidad Nacional de Córdoba. Complejo Astronómico "El Leoncito". Universidad Nacional de la Plata. Complejo Astronómico "El Leoncito". Universidad Nacional de San Juan. Complejo Astronómico "El Leoncito"; Argentina |
description |
Context. The nature of non-variable high-excitation emission lines detected in the optical spectra of normal late-B type and chemically peculiar HgMn and PGa stars is still poorly understood. Aims. To better understand the origin of the weak emission lines in B type stars it is especially important to investigate the spectra of a variety of stars to search for correlations between the emergence of these lines and fundamental stellar parameters. Methods. We have acquired high resolution UVES spectra for the sharp-lined magnetic helium-variable star a Cen over the rotation period of 8.82 d to search for the presence of weak emission lines. Results. For the first time we present observational evidence for the appearance of variable high-excitation Si II, Mn II and Fe II emission lines in a magnetic Bp star. Si II emissions are the strongest at the phase corresponding to the maximum strength of He I lines. Mn II and Fe II emissions vary in antiphase to the He I lines. A correlation is found between the probable location of Mn and Fe surface spots and the strength of the emission lines. On the basis of the currently available data it seems possible that the same kind of selective excitation process is working in the atmospheres of objects within a broad parameter space which could be defined by age, effective temperature, chemical composition, rotational velocity, and magnetic field. Neutral iron lines previously reported to appear broad and shallow at certain phases are not detected in our spectra, although two of them are identified as He I forbidden lines, snowing maximum strength at the phase of the passage of the He rich region across the visible disk. |
publishDate |
2007 |
dc.date.none.fl_str_mv |
2007-12 |
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/11336/213844 Hubrig, S.; Gonzalez, Jorge Federico; Detection of variable Si II, Mn II, and Fe II emission lines in the magnetic Bp star a Centauri; EDP Sciences; Astronomy and Astrophysics; 466; 3; 12-2007; 1083-1087 0004-6361 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/213844 |
identifier_str_mv |
Hubrig, S.; Gonzalez, Jorge Federico; Detection of variable Si II, Mn II, and Fe II emission lines in the magnetic Bp star a Centauri; EDP Sciences; Astronomy and Astrophysics; 466; 3; 12-2007; 1083-1087 0004-6361 CONICET Digital CONICET |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361:20066738 info:eu-repo/semantics/altIdentifier/url/https://www.aanda.org/articles/aa/abs/2007/18/aa6738-06/aa6738-06.html |
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 |
EDP Sciences |
publisher.none.fl_str_mv |
EDP Sciences |
dc.source.none.fl_str_mv |
reponame:CONICET Digital (CONICET) instname:Consejo Nacional de Investigaciones Científicas y Técnicas |
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CONICET Digital (CONICET) |
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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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13.070432 |