The Harmonic Component of the Millihertz Quasi-periodic Oscillations in 4U 1636-53
- Autores
- Fei, Zhenyan; Lyu, Ming; Méndez, Mariano; Altamirano, D.; Zhang, Guobao; Mancuso, Giulio Cesare; Xiang, Fu Yuan; Yang, X. J.
- Año de publicación
- 2021
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- We studied the harmonics of the millihertz quasi-periodic oscillations (mHz QPOs) in the neutron star low-mass X-ray binary 4U 1636-53 using the Rossi X-ray Timing Explorer observations. We detected the harmonics of the mHz QPOs in 73 data intervals, with most of them in the transitional spectra state. We found that the ratio between the rms amplitude of the harmonic and that of the fundamental remains constant in a wide range of the fundamental frequency. More importantly, we studied, for the first time, the rms amplitude of the harmonics versus energy in 4U 1636-53 in the 2-5 keV range. We found that the rms amplitude of both the harmonic and the fundamental shows a decreasing trend as the energy increases, which is different from the behaviors reported in QPOs in certain black hole systems. Furthermore, our results suggest that not all observations with mHz QPOs have the harmonic component, although the reason behind this is still unclear.
Fil: Fei, Zhenyan. Xiangtan University; China
Fil: Lyu, Ming. Xiangtan University; China
Fil: Méndez, Mariano. University of Groningen; Países Bajos
Fil: Altamirano, D.. University of Southampton; Reino Unido
Fil: Zhang, Guobao. Chinese Academy of Sciences; República de China
Fil: Mancuso, Giulio Cesare. Universidad Nacional de La Plata; Argentina. 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
Fil: Xiang, Fu Yuan. Xiangtan University; China
Fil: Yang, X. J.. Xiangtan University; China - Materia
- Low mass X-ray binaries
- Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/158781
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The Harmonic Component of the Millihertz Quasi-periodic Oscillations in 4U 1636-53Fei, ZhenyanLyu, MingMéndez, MarianoAltamirano, D.Zhang, GuobaoMancuso, Giulio CesareXiang, Fu YuanYang, X. J.Low mass X-ray binarieshttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We studied the harmonics of the millihertz quasi-periodic oscillations (mHz QPOs) in the neutron star low-mass X-ray binary 4U 1636-53 using the Rossi X-ray Timing Explorer observations. We detected the harmonics of the mHz QPOs in 73 data intervals, with most of them in the transitional spectra state. We found that the ratio between the rms amplitude of the harmonic and that of the fundamental remains constant in a wide range of the fundamental frequency. More importantly, we studied, for the first time, the rms amplitude of the harmonics versus energy in 4U 1636-53 in the 2-5 keV range. We found that the rms amplitude of both the harmonic and the fundamental shows a decreasing trend as the energy increases, which is different from the behaviors reported in QPOs in certain black hole systems. Furthermore, our results suggest that not all observations with mHz QPOs have the harmonic component, although the reason behind this is still unclear.Fil: Fei, Zhenyan. Xiangtan University; ChinaFil: Lyu, Ming. Xiangtan University; ChinaFil: Méndez, Mariano. University of Groningen; Países BajosFil: Altamirano, D.. University of Southampton; Reino UnidoFil: Zhang, Guobao. Chinese Academy of Sciences; República de ChinaFil: Mancuso, Giulio Cesare. Universidad Nacional de La Plata; Argentina. 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; ArgentinaFil: Xiang, Fu Yuan. Xiangtan University; ChinaFil: Yang, X. J.. Xiangtan University; ChinaIOP Publishing2021-12info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/158781Fei, Zhenyan; Lyu, Ming; Méndez, Mariano; Altamirano, D.; Zhang, Guobao; et al.; The Harmonic Component of the Millihertz Quasi-periodic Oscillations in 4U 1636-53; IOP Publishing; Astrophysical Journal; 922; 2; 12-2021; 119-1300004-637XCONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.3847/1538-4357/ac2501info:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.3847/1538-4357/ac2501info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-10T13:07:52Zoai:ri.conicet.gov.ar:11336/158781instacron: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:34982025-09-10 13:07:52.247CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
The Harmonic Component of the Millihertz Quasi-periodic Oscillations in 4U 1636-53 |
title |
The Harmonic Component of the Millihertz Quasi-periodic Oscillations in 4U 1636-53 |
spellingShingle |
The Harmonic Component of the Millihertz Quasi-periodic Oscillations in 4U 1636-53 Fei, Zhenyan Low mass X-ray binaries |
title_short |
The Harmonic Component of the Millihertz Quasi-periodic Oscillations in 4U 1636-53 |
title_full |
The Harmonic Component of the Millihertz Quasi-periodic Oscillations in 4U 1636-53 |
title_fullStr |
The Harmonic Component of the Millihertz Quasi-periodic Oscillations in 4U 1636-53 |
title_full_unstemmed |
The Harmonic Component of the Millihertz Quasi-periodic Oscillations in 4U 1636-53 |
title_sort |
The Harmonic Component of the Millihertz Quasi-periodic Oscillations in 4U 1636-53 |
dc.creator.none.fl_str_mv |
Fei, Zhenyan Lyu, Ming Méndez, Mariano Altamirano, D. Zhang, Guobao Mancuso, Giulio Cesare Xiang, Fu Yuan Yang, X. J. |
author |
Fei, Zhenyan |
author_facet |
Fei, Zhenyan Lyu, Ming Méndez, Mariano Altamirano, D. Zhang, Guobao Mancuso, Giulio Cesare Xiang, Fu Yuan Yang, X. J. |
author_role |
author |
author2 |
Lyu, Ming Méndez, Mariano Altamirano, D. Zhang, Guobao Mancuso, Giulio Cesare Xiang, Fu Yuan Yang, X. J. |
author2_role |
author author author author author author author |
dc.subject.none.fl_str_mv |
Low mass X-ray binaries |
topic |
Low mass X-ray binaries |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
We studied the harmonics of the millihertz quasi-periodic oscillations (mHz QPOs) in the neutron star low-mass X-ray binary 4U 1636-53 using the Rossi X-ray Timing Explorer observations. We detected the harmonics of the mHz QPOs in 73 data intervals, with most of them in the transitional spectra state. We found that the ratio between the rms amplitude of the harmonic and that of the fundamental remains constant in a wide range of the fundamental frequency. More importantly, we studied, for the first time, the rms amplitude of the harmonics versus energy in 4U 1636-53 in the 2-5 keV range. We found that the rms amplitude of both the harmonic and the fundamental shows a decreasing trend as the energy increases, which is different from the behaviors reported in QPOs in certain black hole systems. Furthermore, our results suggest that not all observations with mHz QPOs have the harmonic component, although the reason behind this is still unclear. Fil: Fei, Zhenyan. Xiangtan University; China Fil: Lyu, Ming. Xiangtan University; China Fil: Méndez, Mariano. University of Groningen; Países Bajos Fil: Altamirano, D.. University of Southampton; Reino Unido Fil: Zhang, Guobao. Chinese Academy of Sciences; República de China Fil: Mancuso, Giulio Cesare. Universidad Nacional de La Plata; Argentina. 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 Fil: Xiang, Fu Yuan. Xiangtan University; China Fil: Yang, X. J.. Xiangtan University; China |
description |
We studied the harmonics of the millihertz quasi-periodic oscillations (mHz QPOs) in the neutron star low-mass X-ray binary 4U 1636-53 using the Rossi X-ray Timing Explorer observations. We detected the harmonics of the mHz QPOs in 73 data intervals, with most of them in the transitional spectra state. We found that the ratio between the rms amplitude of the harmonic and that of the fundamental remains constant in a wide range of the fundamental frequency. More importantly, we studied, for the first time, the rms amplitude of the harmonics versus energy in 4U 1636-53 in the 2-5 keV range. We found that the rms amplitude of both the harmonic and the fundamental shows a decreasing trend as the energy increases, which is different from the behaviors reported in QPOs in certain black hole systems. Furthermore, our results suggest that not all observations with mHz QPOs have the harmonic component, although the reason behind this is still unclear. |
publishDate |
2021 |
dc.date.none.fl_str_mv |
2021-12 |
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/11336/158781 Fei, Zhenyan; Lyu, Ming; Méndez, Mariano; Altamirano, D.; Zhang, Guobao; et al.; The Harmonic Component of the Millihertz Quasi-periodic Oscillations in 4U 1636-53; IOP Publishing; Astrophysical Journal; 922; 2; 12-2021; 119-130 0004-637X CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/158781 |
identifier_str_mv |
Fei, Zhenyan; Lyu, Ming; Méndez, Mariano; Altamirano, D.; Zhang, Guobao; et al.; The Harmonic Component of the Millihertz Quasi-periodic Oscillations in 4U 1636-53; IOP Publishing; Astrophysical Journal; 922; 2; 12-2021; 119-130 0004-637X CONICET Digital CONICET |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/doi/10.3847/1538-4357/ac2501 info:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.3847/1538-4357/ac2501 |
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 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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12.993085 |