BSN: The First Photometric Study of 10 Contact Binary Systems from the Northern and Southern Hemispheres

Autores
Poro, Atila; Li, Kai; Michel, Raul; Castro, Angel; Fernandez Lajus, Eduardo Eusebio; Wang, Li Heng; Coliac, Jean François; Aladağ, Yasemin; Alizadehsabegh, Ailar; Alicavus, Fahri
Año de publicación
2024
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
Photometric observations were made with standard filters in four observatories for 10 contact binary systems. We analyzed the orbital period variations of the systems and found that six of them show long-term changes. The increase in the orbital period of the J07, N65, and PU Vir systems is caused by mass transfer, and the reduction in the orbital period of the J05, LO Psc, and N49 systems is caused by the combination of angular momentum loss and mass transfer. The first light-curve analysis was performed with the PHysics Of Eclipsing BinariEs Python code and Markov Chain Monte Carlo. We discussed the accuracy of photometric mass ratio estimates for contact binary systems with total and partial eclipses compared to spectroscopic results. We also compared our mass ratio findings to a recent method that estimates mass ratios from the light curve’s third derivative. Then, we also discussed this new mass ratio estimate method for photometric data. The systems’ positions were displayed in 18 empirical parameter relationships. According to the light-curve analysis and estimation of absolute parameters, systems BE Mus, J07, J08, N49, and N65 are A subtypes, and the others are W subtypes.
Fil: Poro, Atila. Binary Systems of South and North (BSN) Project; Irán
Fil: Li, Kai. Shandong University; China
Fil: Michel, Raul. Universidad Nacional Autónoma de México; México
Fil: Castro, Angel. Universidad Nacional Autónoma de México; México
Fil: Fernandez Lajus, Eduardo Eusebio. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina
Fil: Wang, Li Heng. Shandong University; China
Fil: Coliac, Jean François. Société Astronomique de France; Francia
Fil: Aladağ, Yasemin. University of Çukurova; Turquía
Fil: Alizadehsabegh, Ailar. University of Tabriz; Irán
Fil: Alicavus, Fahri. Çanakkale Onsekiz Mart University; Turquía
Materia
Close binary stars
CCD photometry
Contact binary stars
Fundamental parameters of stars
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/256857
Acceder
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oai_identifier_str oai:ri.conicet.gov.ar:11336/256857
network_acronym_str CONICETDig
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network_name_str CONICET Digital (CONICET)
spelling BSN: The First Photometric Study of 10 Contact Binary Systems from the Northern and Southern HemispheresPoro, AtilaLi, KaiMichel, RaulCastro, AngelFernandez Lajus, Eduardo EusebioWang, Li HengColiac, Jean FrançoisAladağ, YaseminAlizadehsabegh, AilarAlicavus, FahriClose binary starsCCD photometryContact binary starsFundamental parameters of starshttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Photometric observations were made with standard filters in four observatories for 10 contact binary systems. We analyzed the orbital period variations of the systems and found that six of them show long-term changes. The increase in the orbital period of the J07, N65, and PU Vir systems is caused by mass transfer, and the reduction in the orbital period of the J05, LO Psc, and N49 systems is caused by the combination of angular momentum loss and mass transfer. The first light-curve analysis was performed with the PHysics Of Eclipsing BinariEs Python code and Markov Chain Monte Carlo. We discussed the accuracy of photometric mass ratio estimates for contact binary systems with total and partial eclipses compared to spectroscopic results. We also compared our mass ratio findings to a recent method that estimates mass ratios from the light curve’s third derivative. Then, we also discussed this new mass ratio estimate method for photometric data. The systems’ positions were displayed in 18 empirical parameter relationships. According to the light-curve analysis and estimation of absolute parameters, systems BE Mus, J07, J08, N49, and N65 are A subtypes, and the others are W subtypes.Fil: Poro, Atila. Binary Systems of South and North (BSN) Project; IránFil: Li, Kai. Shandong University; ChinaFil: Michel, Raul. Universidad Nacional Autónoma de México; MéxicoFil: Castro, Angel. Universidad Nacional Autónoma de México; MéxicoFil: Fernandez Lajus, Eduardo Eusebio. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; ArgentinaFil: Wang, Li Heng. Shandong University; ChinaFil: Coliac, Jean François. Société Astronomique de France; FranciaFil: Aladağ, Yasemin. University of Çukurova; TurquíaFil: Alizadehsabegh, Ailar. University of Tabriz; IránFil: Alicavus, Fahri. Çanakkale Onsekiz Mart University; TurquíaIOP Publishing2024-11info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/256857Poro, Atila; Li, Kai; Michel, Raul; Castro, Angel; Fernandez Lajus, Eduardo Eusebio; et al.; BSN: The First Photometric Study of 10 Contact Binary Systems from the Northern and Southern Hemispheres; IOP Publishing; Astronomical Journal; 168; 6; 11-2024; 1-190004-6256CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.3847/1538-3881/ad8345info:eu-repo/semantics/altIdentifier/doi/10.3847/1538-3881/ad8345info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-15T15:37:28Zoai:ri.conicet.gov.ar:11336/256857instacron: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:34982025-10-15 15:37:29.073CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv BSN: The First Photometric Study of 10 Contact Binary Systems from the Northern and Southern Hemispheres
title BSN: The First Photometric Study of 10 Contact Binary Systems from the Northern and Southern Hemispheres
spellingShingle BSN: The First Photometric Study of 10 Contact Binary Systems from the Northern and Southern Hemispheres
Poro, Atila
Close binary stars
CCD photometry
Contact binary stars
Fundamental parameters of stars
title_short BSN: The First Photometric Study of 10 Contact Binary Systems from the Northern and Southern Hemispheres
title_full BSN: The First Photometric Study of 10 Contact Binary Systems from the Northern and Southern Hemispheres
title_fullStr BSN: The First Photometric Study of 10 Contact Binary Systems from the Northern and Southern Hemispheres
title_full_unstemmed BSN: The First Photometric Study of 10 Contact Binary Systems from the Northern and Southern Hemispheres
title_sort BSN: The First Photometric Study of 10 Contact Binary Systems from the Northern and Southern Hemispheres
dc.creator.none.fl_str_mv Poro, Atila
Li, Kai
Michel, Raul
Castro, Angel
Fernandez Lajus, Eduardo Eusebio
Wang, Li Heng
Coliac, Jean François
Aladağ, Yasemin
Alizadehsabegh, Ailar
Alicavus, Fahri
author Poro, Atila
author_facet Poro, Atila
Li, Kai
Michel, Raul
Castro, Angel
Fernandez Lajus, Eduardo Eusebio
Wang, Li Heng
Coliac, Jean François
Aladağ, Yasemin
Alizadehsabegh, Ailar
Alicavus, Fahri
author_role author
author2 Li, Kai
Michel, Raul
Castro, Angel
Fernandez Lajus, Eduardo Eusebio
Wang, Li Heng
Coliac, Jean François
Aladağ, Yasemin
Alizadehsabegh, Ailar
Alicavus, Fahri
author2_role author
author
author
author
author
author
author
author
author
dc.subject.none.fl_str_mv Close binary stars
CCD photometry
Contact binary stars
Fundamental parameters of stars
topic Close binary stars
CCD photometry
Contact binary stars
Fundamental parameters of stars
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv Photometric observations were made with standard filters in four observatories for 10 contact binary systems. We analyzed the orbital period variations of the systems and found that six of them show long-term changes. The increase in the orbital period of the J07, N65, and PU Vir systems is caused by mass transfer, and the reduction in the orbital period of the J05, LO Psc, and N49 systems is caused by the combination of angular momentum loss and mass transfer. The first light-curve analysis was performed with the PHysics Of Eclipsing BinariEs Python code and Markov Chain Monte Carlo. We discussed the accuracy of photometric mass ratio estimates for contact binary systems with total and partial eclipses compared to spectroscopic results. We also compared our mass ratio findings to a recent method that estimates mass ratios from the light curve’s third derivative. Then, we also discussed this new mass ratio estimate method for photometric data. The systems’ positions were displayed in 18 empirical parameter relationships. According to the light-curve analysis and estimation of absolute parameters, systems BE Mus, J07, J08, N49, and N65 are A subtypes, and the others are W subtypes.
Fil: Poro, Atila. Binary Systems of South and North (BSN) Project; Irán
Fil: Li, Kai. Shandong University; China
Fil: Michel, Raul. Universidad Nacional Autónoma de México; México
Fil: Castro, Angel. Universidad Nacional Autónoma de México; México
Fil: Fernandez Lajus, Eduardo Eusebio. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina
Fil: Wang, Li Heng. Shandong University; China
Fil: Coliac, Jean François. Société Astronomique de France; Francia
Fil: Aladağ, Yasemin. University of Çukurova; Turquía
Fil: Alizadehsabegh, Ailar. University of Tabriz; Irán
Fil: Alicavus, Fahri. Çanakkale Onsekiz Mart University; Turquía
description Photometric observations were made with standard filters in four observatories for 10 contact binary systems. We analyzed the orbital period variations of the systems and found that six of them show long-term changes. The increase in the orbital period of the J07, N65, and PU Vir systems is caused by mass transfer, and the reduction in the orbital period of the J05, LO Psc, and N49 systems is caused by the combination of angular momentum loss and mass transfer. The first light-curve analysis was performed with the PHysics Of Eclipsing BinariEs Python code and Markov Chain Monte Carlo. We discussed the accuracy of photometric mass ratio estimates for contact binary systems with total and partial eclipses compared to spectroscopic results. We also compared our mass ratio findings to a recent method that estimates mass ratios from the light curve’s third derivative. Then, we also discussed this new mass ratio estimate method for photometric data. The systems’ positions were displayed in 18 empirical parameter relationships. According to the light-curve analysis and estimation of absolute parameters, systems BE Mus, J07, J08, N49, and N65 are A subtypes, and the others are W subtypes.
publishDate 2024
dc.date.none.fl_str_mv 2024-11
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/11336/256857
Poro, Atila; Li, Kai; Michel, Raul; Castro, Angel; Fernandez Lajus, Eduardo Eusebio; et al.; BSN: The First Photometric Study of 10 Contact Binary Systems from the Northern and Southern Hemispheres; IOP Publishing; Astronomical Journal; 168; 6; 11-2024; 1-19
0004-6256
CONICET Digital
CONICET
url http://hdl.handle.net/11336/256857
identifier_str_mv Poro, Atila; Li, Kai; Michel, Raul; Castro, Angel; Fernandez Lajus, Eduardo Eusebio; et al.; BSN: The First Photometric Study of 10 Contact Binary Systems from the Northern and Southern Hemispheres; IOP Publishing; Astronomical Journal; 168; 6; 11-2024; 1-19
0004-6256
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.3847/1538-3881/ad8345
info:eu-repo/semantics/altIdentifier/doi/10.3847/1538-3881/ad8345
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by/2.5/ar/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by/2.5/ar/
dc.format.none.fl_str_mv application/pdf
application/pdf
dc.publisher.none.fl_str_mv IOP Publishing
publisher.none.fl_str_mv IOP Publishing
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
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score 13.051919

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