Eclipsing Am binary systems in the superWASP survey

Autores
Smalley, B.; Southworth, J.; Pintado, Olga Ines; Gillon, M.; Holdsworth, D. L.; Anderson, D. R.; Barros, S. C. C.; Collier Cameron, A.; Delrez, L.; Faedi, F.; Haswell, C. A.; Hellier, C.; Horne, K.; Jehin, E.; Maxted, P. F. L.; Norton, Andrew; Pollacco, D.; Skillen, I.; Smith, A. M. S.; West, R. G.; Wheatley, P. J.
Año de publicación
2014
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
The results of a search for eclipsing Am star binaries using photometry from the SuperWASP survey are presented. The light curves of 1742 Am stars fainter than V = 8.0 were analysed for the presence of eclipses. A total of 70 stars were found to exhibit eclipses, with 66 having sufficient observations to enable orbital periods to be determined and 28 of which are newly identified eclipsing systems. Also presented are spectroscopic orbits for 5 of the systems. The number of systems and the period distribution is found to be consistent with that identified in previous radial velocity surveys of " classical" Am stars.
Fil: Smalley, B.. Keele University; Reino Unido
Fil: Southworth, J.. Keele University; Reino Unido
Fil: Pintado, Olga Ines. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Tucumán. Instituto Superior de Correlación Geológica. Universidad Nacional de Tucumán. Facultad de Ciencias Naturales e Instituto Miguel Lillo. Departamento de Geología. Cátedra Geología Estructural. Instituto Superior de Correlación Geológica; Argentina
Fil: Gillon, M.. Université de Liege; Bélgica
Fil: Holdsworth, D. L.. Keele University; Reino Unido
Fil: Anderson, D. R.. Keele University; Reino Unido
Fil: Barros, S. C. C.. Aix-Marseille Université; Francia. Centre National de la Recherche Scientifique; Francia
Fil: Collier Cameron, A.. University of St. Andrews; Reino Unido
Fil: Delrez, L.. Université de Liege; Bélgica
Fil: Faedi, F.. University of Warwick; Reino Unido
Fil: Haswell, C. A.. Open University; Reino Unido
Fil: Hellier, C.. Keele University; Reino Unido
Fil: Horne, K.. University of St. Andrews; Reino Unido
Fil: Jehin, E.. Université de Liege; Bélgica
Fil: Maxted, P. F. L.. Keele University; Reino Unido
Fil: Norton, Andrew. Open University; Reino Unido
Fil: Pollacco, D.. University of Warwick; Reino Unido
Fil: Skillen, I.. Isaac Newton Group of Telescopes; España
Fil: Smith, A. M. S.. Polish Academy of Sciences; Argentina
Fil: West, R. G.. University of Warwick; Reino Unido
Fil: Wheatley, P. J.. University of Warwick; Reino Unido
Materia
BINARIES: ECLIPSING
STARS: CHEMICALLY PECULIAR
STARS: EARLY-TYPE
STARS: FUNDAMENTAL PARAMETERS
TECHNIQUES: PHOTOMETRIC
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/37154
Acceder
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oai_identifier_str oai:ri.conicet.gov.ar:11336/37154
network_acronym_str CONICETDig
repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling Eclipsing Am binary systems in the superWASP surveySmalley, B.Southworth, J.Pintado, Olga InesGillon, M.Holdsworth, D. L.Anderson, D. R.Barros, S. C. C.Collier Cameron, A.Delrez, L.Faedi, F.Haswell, C. A.Hellier, C.Horne, K.Jehin, E.Maxted, P. F. L.Norton, AndrewPollacco, D.Skillen, I.Smith, A. M. S.West, R. G.Wheatley, P. J.BINARIES: ECLIPSINGSTARS: CHEMICALLY PECULIARSTARS: EARLY-TYPESTARS: FUNDAMENTAL PARAMETERSTECHNIQUES: PHOTOMETRIChttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1The results of a search for eclipsing Am star binaries using photometry from the SuperWASP survey are presented. The light curves of 1742 Am stars fainter than V = 8.0 were analysed for the presence of eclipses. A total of 70 stars were found to exhibit eclipses, with 66 having sufficient observations to enable orbital periods to be determined and 28 of which are newly identified eclipsing systems. Also presented are spectroscopic orbits for 5 of the systems. The number of systems and the period distribution is found to be consistent with that identified in previous radial velocity surveys of " classical" Am stars.Fil: Smalley, B.. Keele University; Reino UnidoFil: Southworth, J.. Keele University; Reino UnidoFil: Pintado, Olga Ines. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Tucumán. Instituto Superior de Correlación Geológica. Universidad Nacional de Tucumán. Facultad de Ciencias Naturales e Instituto Miguel Lillo. Departamento de Geología. Cátedra Geología Estructural. Instituto Superior de Correlación Geológica; ArgentinaFil: Gillon, M.. Université de Liege; BélgicaFil: Holdsworth, D. L.. Keele University; Reino UnidoFil: Anderson, D. R.. Keele University; Reino UnidoFil: Barros, S. C. C.. Aix-Marseille Université; Francia. Centre National de la Recherche Scientifique; FranciaFil: Collier Cameron, A.. University of St. Andrews; Reino UnidoFil: Delrez, L.. Université de Liege; BélgicaFil: Faedi, F.. University of Warwick; Reino UnidoFil: Haswell, C. A.. Open University; Reino UnidoFil: Hellier, C.. Keele University; Reino UnidoFil: Horne, K.. University of St. Andrews; Reino UnidoFil: Jehin, E.. Université de Liege; BélgicaFil: Maxted, P. F. L.. Keele University; Reino UnidoFil: Norton, Andrew. Open University; Reino UnidoFil: Pollacco, D.. University of Warwick; Reino UnidoFil: Skillen, I.. Isaac Newton Group of Telescopes; EspañaFil: Smith, A. M. S.. Polish Academy of Sciences; ArgentinaFil: West, R. G.. University of Warwick; Reino UnidoFil: Wheatley, P. J.. University of Warwick; Reino UnidoEDP Sciences2014-04info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/37154Smalley, B.; Southworth, J.; Pintado, Olga Ines; Gillon, M.; Holdsworth, D. L.; et al.; Eclipsing Am binary systems in the superWASP survey; EDP Sciences; Astronomy and Astrophysics; 564; 4-2014; 69-890004-6361CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361/201323158info:eu-repo/semantics/altIdentifier/url/https://www.aanda.org/articles/aa/abs/2014/04/aa23158-13/aa23158-13.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 Técnicas2025-09-17T10:47:25Zoai:ri.conicet.gov.ar:11336/37154instacron: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:34982025-09-17 10:47:25.753CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Eclipsing Am binary systems in the superWASP survey
title Eclipsing Am binary systems in the superWASP survey
spellingShingle Eclipsing Am binary systems in the superWASP survey
Smalley, B.
BINARIES: ECLIPSING
STARS: CHEMICALLY PECULIAR
STARS: EARLY-TYPE
STARS: FUNDAMENTAL PARAMETERS
TECHNIQUES: PHOTOMETRIC
title_short Eclipsing Am binary systems in the superWASP survey
title_full Eclipsing Am binary systems in the superWASP survey
title_fullStr Eclipsing Am binary systems in the superWASP survey
title_full_unstemmed Eclipsing Am binary systems in the superWASP survey
title_sort Eclipsing Am binary systems in the superWASP survey
dc.creator.none.fl_str_mv Smalley, B.
Southworth, J.
Pintado, Olga Ines
Gillon, M.
Holdsworth, D. L.
Anderson, D. R.
Barros, S. C. C.
Collier Cameron, A.
Delrez, L.
Faedi, F.
Haswell, C. A.
Hellier, C.
Horne, K.
Jehin, E.
Maxted, P. F. L.
Norton, Andrew
Pollacco, D.
Skillen, I.
Smith, A. M. S.
West, R. G.
Wheatley, P. J.
author Smalley, B.
author_facet Smalley, B.
Southworth, J.
Pintado, Olga Ines
Gillon, M.
Holdsworth, D. L.
Anderson, D. R.
Barros, S. C. C.
Collier Cameron, A.
Delrez, L.
Faedi, F.
Haswell, C. A.
Hellier, C.
Horne, K.
Jehin, E.
Maxted, P. F. L.
Norton, Andrew
Pollacco, D.
Skillen, I.
Smith, A. M. S.
West, R. G.
Wheatley, P. J.
author_role author
author2 Southworth, J.
Pintado, Olga Ines
Gillon, M.
Holdsworth, D. L.
Anderson, D. R.
Barros, S. C. C.
Collier Cameron, A.
Delrez, L.
Faedi, F.
Haswell, C. A.
Hellier, C.
Horne, K.
Jehin, E.
Maxted, P. F. L.
Norton, Andrew
Pollacco, D.
Skillen, I.
Smith, A. M. S.
West, R. G.
Wheatley, P. J.
author2_role author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
dc.subject.none.fl_str_mv BINARIES: ECLIPSING
STARS: CHEMICALLY PECULIAR
STARS: EARLY-TYPE
STARS: FUNDAMENTAL PARAMETERS
TECHNIQUES: PHOTOMETRIC
topic BINARIES: ECLIPSING
STARS: CHEMICALLY PECULIAR
STARS: EARLY-TYPE
STARS: FUNDAMENTAL PARAMETERS
TECHNIQUES: PHOTOMETRIC
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv The results of a search for eclipsing Am star binaries using photometry from the SuperWASP survey are presented. The light curves of 1742 Am stars fainter than V = 8.0 were analysed for the presence of eclipses. A total of 70 stars were found to exhibit eclipses, with 66 having sufficient observations to enable orbital periods to be determined and 28 of which are newly identified eclipsing systems. Also presented are spectroscopic orbits for 5 of the systems. The number of systems and the period distribution is found to be consistent with that identified in previous radial velocity surveys of " classical" Am stars.
Fil: Smalley, B.. Keele University; Reino Unido
Fil: Southworth, J.. Keele University; Reino Unido
Fil: Pintado, Olga Ines. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Tucumán. Instituto Superior de Correlación Geológica. Universidad Nacional de Tucumán. Facultad de Ciencias Naturales e Instituto Miguel Lillo. Departamento de Geología. Cátedra Geología Estructural. Instituto Superior de Correlación Geológica; Argentina
Fil: Gillon, M.. Université de Liege; Bélgica
Fil: Holdsworth, D. L.. Keele University; Reino Unido
Fil: Anderson, D. R.. Keele University; Reino Unido
Fil: Barros, S. C. C.. Aix-Marseille Université; Francia. Centre National de la Recherche Scientifique; Francia
Fil: Collier Cameron, A.. University of St. Andrews; Reino Unido
Fil: Delrez, L.. Université de Liege; Bélgica
Fil: Faedi, F.. University of Warwick; Reino Unido
Fil: Haswell, C. A.. Open University; Reino Unido
Fil: Hellier, C.. Keele University; Reino Unido
Fil: Horne, K.. University of St. Andrews; Reino Unido
Fil: Jehin, E.. Université de Liege; Bélgica
Fil: Maxted, P. F. L.. Keele University; Reino Unido
Fil: Norton, Andrew. Open University; Reino Unido
Fil: Pollacco, D.. University of Warwick; Reino Unido
Fil: Skillen, I.. Isaac Newton Group of Telescopes; España
Fil: Smith, A. M. S.. Polish Academy of Sciences; Argentina
Fil: West, R. G.. University of Warwick; Reino Unido
Fil: Wheatley, P. J.. University of Warwick; Reino Unido
description The results of a search for eclipsing Am star binaries using photometry from the SuperWASP survey are presented. The light curves of 1742 Am stars fainter than V = 8.0 were analysed for the presence of eclipses. A total of 70 stars were found to exhibit eclipses, with 66 having sufficient observations to enable orbital periods to be determined and 28 of which are newly identified eclipsing systems. Also presented are spectroscopic orbits for 5 of the systems. The number of systems and the period distribution is found to be consistent with that identified in previous radial velocity surveys of " classical" Am stars.
publishDate 2014
dc.date.none.fl_str_mv 2014-04
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/11336/37154
Smalley, B.; Southworth, J.; Pintado, Olga Ines; Gillon, M.; Holdsworth, D. L.; et al.; Eclipsing Am binary systems in the superWASP survey; EDP Sciences; Astronomy and Astrophysics; 564; 4-2014; 69-89
0004-6361
CONICET Digital
CONICET
url http://hdl.handle.net/11336/37154
identifier_str_mv Smalley, B.; Southworth, J.; Pintado, Olga Ines; Gillon, M.; Holdsworth, D. L.; et al.; Eclipsing Am binary systems in the superWASP survey; EDP Sciences; Astronomy and Astrophysics; 564; 4-2014; 69-89
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/10.1051/0004-6361/201323158
info:eu-repo/semantics/altIdentifier/url/https://www.aanda.org/articles/aa/abs/2014/04/aa23158-13/aa23158-13.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
reponame_str CONICET Digital (CONICET)
collection 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
_version_ 1843606059101454336
score 13.001348

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