Ten CoRoT eclipsing binaries: photometric solutions
Autor(a) principal: | |
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Data de Publicação: | 2011 |
Outros Autores: | , |
Tipo de documento: | Artigo |
Idioma: | eng |
Título da fonte: | Repositório Institucional da UFRN |
Texto Completo: | https://repositorio.ufrn.br/jspui/handle/123456789/29107 https://doi.org/10.1016/j.newast.2010.07.006 |
Resumo: | Ten eclipsing binaries, identified in the scope of the CoRoT Space Mission, were selected for analysis. The photometric light curves were processed and analyzed, resulting in the first study of eclipsing binary candidates with their possible photometric solution, in the context of the above-mentioned Space Mission. The selected targets are detached and overcontact systems, for which we computed 2MASS temperatures, in addition to different physical parameters, including orbital period, orbit inclination angle, and temperatures, radius and luminosity ratios. This study reveals a large diversity of eclipsing binary systems obtained from the CoRoT data. |
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Maciel, S.COsorio, Y.F.MMedeiros, José Renan de2020-05-31T23:28:30Z2020-05-31T23:28:30Z2011Maciel, S.C. ; Osorio, Y.F.M. ; De Medeiros, J.R. . Ten CoRoT eclipsing binaries: photometric solutions?. New Astronomy (Gedrukt), v. 16, p. 68-71, 2011. Disponível em: https://www.sciencedirect.com/science/article/pii/S1384107610000849?via%3Dihub. Acesso em: 25 Maio 2020. https://doi.org/10.1016/j.newast.2010.07.006https://repositorio.ufrn.br/jspui/handle/123456789/29107https://doi.org/10.1016/j.newast.2010.07.006ELSEVIERAttribution-NonCommercial-NoDerivs 3.0 Brazilhttp://creativecommons.org/licenses/by-nc-nd/3.0/br/info:eu-repo/semantics/openAccessStar; CoRoT; Eclipsing binaries; Fundamental parametersTen CoRoT eclipsing binaries: photometric solutionsinfo:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articleTen eclipsing binaries, identified in the scope of the CoRoT Space Mission, were selected for analysis. The photometric light curves were processed and analyzed, resulting in the first study of eclipsing binary candidates with their possible photometric solution, in the context of the above-mentioned Space Mission. The selected targets are detached and overcontact systems, for which we computed 2MASS temperatures, in addition to different physical parameters, including orbital period, orbit inclination angle, and temperatures, radius and luminosity ratios. This study reveals a large diversity of eclipsing binary systems obtained from the CoRoT data.engreponame:Repositório Institucional da UFRNinstname:Universidade Federal do Rio Grande do Norte (UFRN)instacron:UFRNORIGINALTenCoRoTEclipsingBinariesPhotometricSolution_Medeiros_2011.pdfTenCoRoTEclipsingBinariesPhotometricSolution_Medeiros_2011.pdfapplication/pdf936470https://repositorio.ufrn.br/bitstream/123456789/29107/1/TenCoRoTEclipsingBinariesPhotometricSolution_Medeiros_2011.pdf8c6b9435450d597821e9c7e9624ae91cMD51CC-LICENSElicense_rdflicense_rdfapplication/rdf+xml; charset=utf-8811https://repositorio.ufrn.br/bitstream/123456789/29107/2/license_rdfe39d27027a6cc9cb039ad269a5db8e34MD52LICENSElicense.txtlicense.txttext/plain; charset=utf-81484https://repositorio.ufrn.br/bitstream/123456789/29107/3/license.txte9597aa2854d128fd968be5edc8a28d9MD53TEXTTenCoRoTEclipsingBinariesPhotometricSolution_Medeiros_2011.pdf.txtTenCoRoTEclipsingBinariesPhotometricSolution_Medeiros_2011.pdf.txtExtracted texttext/plain14264https://repositorio.ufrn.br/bitstream/123456789/29107/4/TenCoRoTEclipsingBinariesPhotometricSolution_Medeiros_2011.pdf.txtf8288d1249356fc7aedfee504fb83d9aMD54THUMBNAILTenCoRoTEclipsingBinariesPhotometricSolution_Medeiros_2011.pdf.jpgTenCoRoTEclipsingBinariesPhotometricSolution_Medeiros_2011.pdf.jpgGenerated Thumbnailimage/jpeg1698https://repositorio.ufrn.br/bitstream/123456789/29107/5/TenCoRoTEclipsingBinariesPhotometricSolution_Medeiros_2011.pdf.jpg5f64acfbc160c68577128630f0abc7e9MD55123456789/291072020-06-07 04:36:12.835oai:https://repositorio.ufrn.br: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Repositório de PublicaçõesPUBhttp://repositorio.ufrn.br/oai/opendoar:2020-06-07T07:36:12Repositório Institucional da UFRN - Universidade Federal do Rio Grande do Norte (UFRN)false |
dc.title.pt_BR.fl_str_mv |
Ten CoRoT eclipsing binaries: photometric solutions |
title |
Ten CoRoT eclipsing binaries: photometric solutions |
spellingShingle |
Ten CoRoT eclipsing binaries: photometric solutions Maciel, S.C Star; CoRoT; Eclipsing binaries; Fundamental parameters |
title_short |
Ten CoRoT eclipsing binaries: photometric solutions |
title_full |
Ten CoRoT eclipsing binaries: photometric solutions |
title_fullStr |
Ten CoRoT eclipsing binaries: photometric solutions |
title_full_unstemmed |
Ten CoRoT eclipsing binaries: photometric solutions |
title_sort |
Ten CoRoT eclipsing binaries: photometric solutions |
author |
Maciel, S.C |
author_facet |
Maciel, S.C Osorio, Y.F.M Medeiros, José Renan de |
author_role |
author |
author2 |
Osorio, Y.F.M Medeiros, José Renan de |
author2_role |
author author |
dc.contributor.author.fl_str_mv |
Maciel, S.C Osorio, Y.F.M Medeiros, José Renan de |
dc.subject.por.fl_str_mv |
Star; CoRoT; Eclipsing binaries; Fundamental parameters |
topic |
Star; CoRoT; Eclipsing binaries; Fundamental parameters |
description |
Ten eclipsing binaries, identified in the scope of the CoRoT Space Mission, were selected for analysis. The photometric light curves were processed and analyzed, resulting in the first study of eclipsing binary candidates with their possible photometric solution, in the context of the above-mentioned Space Mission. The selected targets are detached and overcontact systems, for which we computed 2MASS temperatures, in addition to different physical parameters, including orbital period, orbit inclination angle, and temperatures, radius and luminosity ratios. This study reveals a large diversity of eclipsing binary systems obtained from the CoRoT data. |
publishDate |
2011 |
dc.date.issued.fl_str_mv |
2011 |
dc.date.accessioned.fl_str_mv |
2020-05-31T23:28:30Z |
dc.date.available.fl_str_mv |
2020-05-31T23:28:30Z |
dc.type.status.fl_str_mv |
info:eu-repo/semantics/publishedVersion |
dc.type.driver.fl_str_mv |
info:eu-repo/semantics/article |
format |
article |
status_str |
publishedVersion |
dc.identifier.citation.fl_str_mv |
Maciel, S.C. ; Osorio, Y.F.M. ; De Medeiros, J.R. . Ten CoRoT eclipsing binaries: photometric solutions?. New Astronomy (Gedrukt), v. 16, p. 68-71, 2011. Disponível em: https://www.sciencedirect.com/science/article/pii/S1384107610000849?via%3Dihub. Acesso em: 25 Maio 2020. https://doi.org/10.1016/j.newast.2010.07.006 |
dc.identifier.uri.fl_str_mv |
https://repositorio.ufrn.br/jspui/handle/123456789/29107 |
dc.identifier.doi.none.fl_str_mv |
https://doi.org/10.1016/j.newast.2010.07.006 |
identifier_str_mv |
Maciel, S.C. ; Osorio, Y.F.M. ; De Medeiros, J.R. . Ten CoRoT eclipsing binaries: photometric solutions?. New Astronomy (Gedrukt), v. 16, p. 68-71, 2011. Disponível em: https://www.sciencedirect.com/science/article/pii/S1384107610000849?via%3Dihub. Acesso em: 25 Maio 2020. https://doi.org/10.1016/j.newast.2010.07.006 |
url |
https://repositorio.ufrn.br/jspui/handle/123456789/29107 https://doi.org/10.1016/j.newast.2010.07.006 |
dc.language.iso.fl_str_mv |
eng |
language |
eng |
dc.rights.driver.fl_str_mv |
Attribution-NonCommercial-NoDerivs 3.0 Brazil http://creativecommons.org/licenses/by-nc-nd/3.0/br/ info:eu-repo/semantics/openAccess |
rights_invalid_str_mv |
Attribution-NonCommercial-NoDerivs 3.0 Brazil http://creativecommons.org/licenses/by-nc-nd/3.0/br/ |
eu_rights_str_mv |
openAccess |
dc.publisher.none.fl_str_mv |
ELSEVIER |
publisher.none.fl_str_mv |
ELSEVIER |
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Universidade Federal do Rio Grande do Norte (UFRN) |
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UFRN |
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UFRN |
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Repositório Institucional da UFRN |
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Repositório Institucional da UFRN |
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