The δ scuti star FG vir. V. The 2002 photometric multisite campaign

A high-accuracy multisite campaign was carried out from 2002 January to May with a photometric coverage of 398 h at five observatories. The concentration on a few selected sites gives better consistency and accuracy than collecting smaller amounts from a larger number of sites. 23 frequencies were d...

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Autores: Breger, M., Rodler, F., Pretorius, M. L., Martín, Susana, Amado, Pedro J., Costa, Víctor M., Rodríguez Martínez, Eloy, Garrido, Rafael, López de Coca, Pilar, Olivares, I., Rolland, Ángel, Tshenye, T., Handler, G., Poretti, Ennio, Sareyan, J. P., Álvarez, Manuel Antonio, Kilmartin, P., Zima, W.
Tipo de recurso: artículo
Estado:Versión publicada
Fecha de publicación:2004
País:España
Institución:Consejo Superior de Investigaciones Científicas (CSIC)
Repositorio:DIGITAL.CSIC. Repositorio Institucional del CSIC
OAI Identifier:oai:digital.csic.es:10261/226843
Acceso en línea:http://hdl.handle.net/10261/226843
Access Level:acceso abierto
Palabra clave:Stars: variables: δ Sct
Stars: oscillations
Stars: individual: FG Vir
Techniques: photometric
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spelling The δ scuti star FG vir. V. The 2002 photometric multisite campaignBreger, M.Rodler, F.Pretorius, M. L.Martín, SusanaAmado, Pedro J.Costa, Víctor M.Rodríguez Martínez, EloyGarrido, RafaelLópez de Coca, PilarOlivares, I.Rolland, ÁngelTshenye, T.Handler, G.Poretti, EnnioSareyan, J. P.Álvarez, Manuel AntonioKilmartin, P.Zima, W.Stars: variables: δ SctStars: oscillationsStars: individual: FG VirTechniques: photometricA high-accuracy multisite campaign was carried out from 2002 January to May with a photometric coverage of 398 h at five observatories. The concentration on a few selected sites gives better consistency and accuracy than collecting smaller amounts from a larger number of sites. 23 frequencies were detected with a high statistical significance. 6 of these are new. The 17 frequencies found in common with the 1992-1995 data are the modes with highest amplitudes. This indicates that the pulsation spectrum of FG Vir is relatively stable over the ten-year period. Two frequencies have variable amplitudes and phases from year to year as well as during 2002. These were both found to be double modes with close frequencies. For the mode at 12.15 c/d this leads to an apparent modulation with a time scale of ∼ 129 d. The close frequencies at 12.15 c/d are composed of a radial and a nonradial mode, suggesting a similarity with the Blazhko Effect seen in RR Lyrae stars.This investigation has been supported by the Austrian Fonds zur Förderung der wissenschaftlichen Forschung, project number P14546-PHY. The Sierra Nevada observations were supported by the Junta de Andalucia and the DGI under project AYA2000-1580. P.J.A. acknowledges financial support at the Instituto de Astrofísica de Andalucía-CSIC by an I3P contract (I3P-PC2001-1) funded by the European Social Fund. S.M.R. also acknowledge the financial support by a Marie Curie Fellowship of the European Community programme ’Improving the Human Potential’ under contract number HPMF-CT-2001-01146.EDP SciencesAustrian Science FundJunta de AndalucíaDirección General de Investigación Científica y Técnica, DGICT (España)Consejo Superior de Investigaciones Científicas (España)European CommissionConsejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]2021202120042021info:eu-repo/semantics/articlehttp://purl.org/coar/resource_type/c_6501Publisher's versioninfo:eu-repo/semantics/publishedVersionhttp://hdl.handle.net/10261/226843reponame:DIGITAL.CSIC. Repositorio Institucional del CSICinstname:Consejo Superior de Investigaciones Científicas (CSIC)Ingléshttp://doi.org/10.1051/0004-6361:20035830Síinfo:eu-repo/semantics/openAccessoai:digital.csic.es:10261/2268432026-05-22T06:33:51Z
dc.title.none.fl_str_mv The δ scuti star FG vir. V. The 2002 photometric multisite campaign
title The δ scuti star FG vir. V. The 2002 photometric multisite campaign
spellingShingle The δ scuti star FG vir. V. The 2002 photometric multisite campaign
Breger, M.
Stars: variables: δ Sct
Stars: oscillations
Stars: individual: FG Vir
Techniques: photometric
title_short The δ scuti star FG vir. V. The 2002 photometric multisite campaign
title_full The δ scuti star FG vir. V. The 2002 photometric multisite campaign
title_fullStr The δ scuti star FG vir. V. The 2002 photometric multisite campaign
title_full_unstemmed The δ scuti star FG vir. V. The 2002 photometric multisite campaign
title_sort The δ scuti star FG vir. V. The 2002 photometric multisite campaign
dc.creator.none.fl_str_mv Breger, M.
Rodler, F.
Pretorius, M. L.
Martín, Susana
Amado, Pedro J.
Costa, Víctor M.
Rodríguez Martínez, Eloy
Garrido, Rafael
López de Coca, Pilar
Olivares, I.
Rolland, Ángel
Tshenye, T.
Handler, G.
Poretti, Ennio
Sareyan, J. P.
Álvarez, Manuel Antonio
Kilmartin, P.
Zima, W.
author Breger, M.
author_facet Breger, M.
Rodler, F.
Pretorius, M. L.
Martín, Susana
Amado, Pedro J.
Costa, Víctor M.
Rodríguez Martínez, Eloy
Garrido, Rafael
López de Coca, Pilar
Olivares, I.
Rolland, Ángel
Tshenye, T.
Handler, G.
Poretti, Ennio
Sareyan, J. P.
Álvarez, Manuel Antonio
Kilmartin, P.
Zima, W.
author_role author
author2 Rodler, F.
Pretorius, M. L.
Martín, Susana
Amado, Pedro J.
Costa, Víctor M.
Rodríguez Martínez, Eloy
Garrido, Rafael
López de Coca, Pilar
Olivares, I.
Rolland, Ángel
Tshenye, T.
Handler, G.
Poretti, Ennio
Sareyan, J. P.
Álvarez, Manuel Antonio
Kilmartin, P.
Zima, W.
author2_role author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
dc.contributor.none.fl_str_mv Austrian Science Fund
Junta de Andalucía
Dirección General de Investigación Científica y Técnica, DGICT (España)
Consejo Superior de Investigaciones Científicas (España)
European Commission
Consejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]
dc.subject.none.fl_str_mv Stars: variables: δ Sct
Stars: oscillations
Stars: individual: FG Vir
Techniques: photometric
topic Stars: variables: δ Sct
Stars: oscillations
Stars: individual: FG Vir
Techniques: photometric
description A high-accuracy multisite campaign was carried out from 2002 January to May with a photometric coverage of 398 h at five observatories. The concentration on a few selected sites gives better consistency and accuracy than collecting smaller amounts from a larger number of sites. 23 frequencies were detected with a high statistical significance. 6 of these are new. The 17 frequencies found in common with the 1992-1995 data are the modes with highest amplitudes. This indicates that the pulsation spectrum of FG Vir is relatively stable over the ten-year period. Two frequencies have variable amplitudes and phases from year to year as well as during 2002. These were both found to be double modes with close frequencies. For the mode at 12.15 c/d this leads to an apparent modulation with a time scale of ∼ 129 d. The close frequencies at 12.15 c/d are composed of a radial and a nonradial mode, suggesting a similarity with the Blazhko Effect seen in RR Lyrae stars.
publishDate 2004
dc.date.none.fl_str_mv 2004
2021
2021
2021
dc.type.none.fl_str_mv info:eu-repo/semantics/article
http://purl.org/coar/resource_type/c_6501
Publisher's version
info:eu-repo/semantics/publishedVersion
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://hdl.handle.net/10261/226843
url http://hdl.handle.net/10261/226843
dc.language.none.fl_str_mv Inglés
language_invalid_str_mv Inglés
dc.relation.none.fl_str_mv http://doi.org/10.1051/0004-6361:20035830

dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.publisher.none.fl_str_mv EDP Sciences
publisher.none.fl_str_mv EDP Sciences
dc.source.none.fl_str_mv reponame:DIGITAL.CSIC. Repositorio Institucional del CSIC
instname:Consejo Superior de Investigaciones Científicas (CSIC)
instname_str Consejo Superior de Investigaciones Científicas (CSIC)
reponame_str DIGITAL.CSIC. Repositorio Institucional del CSIC
collection DIGITAL.CSIC. Repositorio Institucional del CSIC
repository.name.fl_str_mv
repository.mail.fl_str_mv
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