A periodicity analysis of the optical variations of 3C 273

Autores
Fan, Jun Hui; Romero, Gustavo Esteban; Rui Guang, Lin
Año de publicación
2001
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
The authors have compiled measurements of N 110 years in the Bband of the quasar 3C 273 and used this database to search for periodicity signals in the optical light curve. Two different methods were applied: the Jurkevich method and the discrete correlation function (DCF) method. They revealed the existence of periods of 2.0, (13.65 f 0.20) and (22.50 f 0.20)yr in the source variability. Possible origin of such a variability is discussed.
Fil: Fan, Jun Hui. Guangzhou University; China
Fil: Romero, Gustavo Esteban. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina. Universidad Nacional de La Plata. Facultad de Ciencias Exactas. Departamento de Física; Argentina
Fil: Rui Guang, Lin. Guangzhou University; China
Materia
Quasars
Active Galaxies
3c 273 (Cuásar)
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:11336/39889
Acceder
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network_name_str CONICET Digital (CONICET)
spelling A periodicity analysis of the optical variations of 3C 273Fan, Jun HuiRomero, Gustavo EstebanRui Guang, LinQuasarsActive Galaxies3c 273 (Cuásar)https://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1The authors have compiled measurements of N 110 years in the Bband of the quasar 3C 273 and used this database to search for periodicity signals in the optical light curve. Two different methods were applied: the Jurkevich method and the discrete correlation function (DCF) method. They revealed the existence of periods of 2.0, (13.65 f 0.20) and (22.50 f 0.20)yr in the source variability. Possible origin of such a variability is discussed.Fil: Fan, Jun Hui. Guangzhou University; ChinaFil: Romero, Gustavo Esteban. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina. Universidad Nacional de La Plata. Facultad de Ciencias Exactas. Departamento de Física; ArgentinaFil: Rui Guang, Lin. Guangzhou University; ChinaElsevier2001-12info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/39889Fan, Jun Hui; Romero, Gustavo Esteban; Rui Guang, Lin; A periodicity analysis of the optical variations of 3C 273; Elsevier; Chinese Astronomy and Astrophysics; 25; 12-2001; 282-2900275-1062CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1016/S0275-1062(01)00076-5info:eu-repo/semantics/altIdentifier/url/https://www.sciencedirect.com/science/article/pii/S0275106201000765info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-22T11:52:44Zoai:ri.conicet.gov.ar:11336/39889instacron: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:34982025-10-22 11:52:44.662CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv A periodicity analysis of the optical variations of 3C 273
title A periodicity analysis of the optical variations of 3C 273
spellingShingle A periodicity analysis of the optical variations of 3C 273
Fan, Jun Hui
Quasars
Active Galaxies
3c 273 (Cuásar)
title_short A periodicity analysis of the optical variations of 3C 273
title_full A periodicity analysis of the optical variations of 3C 273
title_fullStr A periodicity analysis of the optical variations of 3C 273
title_full_unstemmed A periodicity analysis of the optical variations of 3C 273
title_sort A periodicity analysis of the optical variations of 3C 273
dc.creator.none.fl_str_mv Fan, Jun Hui
Romero, Gustavo Esteban
Rui Guang, Lin
author Fan, Jun Hui
author_facet Fan, Jun Hui
Romero, Gustavo Esteban
Rui Guang, Lin
author_role author
author2 Romero, Gustavo Esteban
Rui Guang, Lin
author2_role author
author
dc.subject.none.fl_str_mv Quasars
Active Galaxies
3c 273 (Cuásar)
topic Quasars
Active Galaxies
3c 273 (Cuásar)
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 authors have compiled measurements of N 110 years in the Bband of the quasar 3C 273 and used this database to search for periodicity signals in the optical light curve. Two different methods were applied: the Jurkevich method and the discrete correlation function (DCF) method. They revealed the existence of periods of 2.0, (13.65 f 0.20) and (22.50 f 0.20)yr in the source variability. Possible origin of such a variability is discussed.
Fil: Fan, Jun Hui. Guangzhou University; China
Fil: Romero, Gustavo Esteban. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina. Universidad Nacional de La Plata. Facultad de Ciencias Exactas. Departamento de Física; Argentina
Fil: Rui Guang, Lin. Guangzhou University; China
description The authors have compiled measurements of N 110 years in the Bband of the quasar 3C 273 and used this database to search for periodicity signals in the optical light curve. Two different methods were applied: the Jurkevich method and the discrete correlation function (DCF) method. They revealed the existence of periods of 2.0, (13.65 f 0.20) and (22.50 f 0.20)yr in the source variability. Possible origin of such a variability is discussed.
publishDate 2001
dc.date.none.fl_str_mv 2001-12
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/11336/39889
Fan, Jun Hui; Romero, Gustavo Esteban; Rui Guang, Lin; A periodicity analysis of the optical variations of 3C 273; Elsevier; Chinese Astronomy and Astrophysics; 25; 12-2001; 282-290
0275-1062
CONICET Digital
CONICET
url http://hdl.handle.net/11336/39889
identifier_str_mv Fan, Jun Hui; Romero, Gustavo Esteban; Rui Guang, Lin; A periodicity analysis of the optical variations of 3C 273; Elsevier; Chinese Astronomy and Astrophysics; 25; 12-2001; 282-290
0275-1062
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/doi/10.1016/S0275-1062(01)00076-5
info:eu-repo/semantics/altIdentifier/url/https://www.sciencedirect.com/science/article/pii/S0275106201000765
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 Elsevier
publisher.none.fl_str_mv Elsevier
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_ 1846782220552896512
score 12.928904

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