Fast transitions of X-ray variability in the black hole transient GX 339−4: comparison with MAXI J1820+070 and MAXI J1348−630

Autores: Yang, Zi Xu; Zhang, Liang; Zhang, S. N.; Méndez, M.; García, Federico; Huang, Yue; Bu, Qingcui; Liu, He Xin; Yu, Wei; Wang, P. J.; Tao, L.; Altamirano, D.; Qu, Jin Lu; Zhang, S.; Ma, X.; Song, L. M.; Jia, S. M.; Ge, M. Y.; Liu, Q. Z.; Yan, J. Z.; Li, T. M.; Ren, X. Q.; Ma, R. C.; Zhang, Yuexin; Zhou, Xudong; Ma, B. Y.; Du, Y. F.; Fu, Y. C.; Xiao, Y. X.; Li, P. P.; Jin, P.; Zhao, S. J.; Zhao, Q. C.
Año de publicación: 2023
Idioma: inglés
Tipo de recurso: artículo
Estado: versión publicada
Descripción: Fast transitions between different types of power density spectra (PDS) happening over time-scales of several tens of seconds are rare phenomena in black hole X-ray binaries. In this paper, we report a broad-band spectral-timing analysis of the fast transitions observed in the 2021 outburst of GX 339-4 using NICER and Insight-HXMT observations. We observe transitions between band-limited noise-dominated PDS and type-B quasi-periodic oscillations (QPOs), and their rapid appearance or disappearance. We also make a detailed comparison between the fast transitions in GX 339-4 with those seen in MAXI J1820+070 and MAXI J1348-630. By comparing the spectra of the periods with and without type-B QPOs, we find that the spectral ratios above 10 keV are nearly constant or slightly decreasing, and the values are different between sources. Below 10 keV, the flux change of the Comptonization component is inversely proportional to the flux change of the thermal component, suggesting that the appearance of type-B QPOs is associated with a redistribution of the accretion power between the disc and the Comptonizing emission region. The spectral ratios between the periods with type-B QPO and those with broad-band noise are significantly different from that with type-B QPO and without type-B QPO, where the ratios (type-B QPO/broad-band noise) show a maximum at around 4 keV and then decrease gradually towards high energies. Finally, we discuss the possible change of the geometry of the inner accretion flow and/or jet during the transitions.
Fil: Yang, Zi Xu. Chinese Academy of Sciences; República de China
Fil: Zhang, Liang. Chinese Academy of Sciences; República de China
Fil: Zhang, S. N.. Chinese Academy of Sciences; República de China
Fil: Méndez, M.. Kapteyn Astronomical Institute; Países Bajos
Fil: García, Federico. 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: Huang, Yue. Chinese Academy of Sciences; República de China
Fil: Bu, Qingcui. Eberhard Karls Universität Tübingen; Alemania
Fil: Liu, He Xin. Chinese Academy of Sciences; República de China
Fil: Yu, Wei. Chinese Academy of Sciences; República de China
Fil: Wang, P. J.. Chinese Academy of Sciences; República de China
Fil: Tao, L.. Chinese Academy of Sciences; República de China
Fil: Altamirano, D.. University of Southampton; Reino Unido
Fil: Qu, Jin Lu. Chinese Academy of Sciences; República de China
Fil: Zhang, S.. Chinese Academy of Sciences; República de China
Fil: Ma, X.. Chinese Academy of Sciences; República de China
Fil: Song, L. M.. Chinese Academy of Sciences; República de China
Fil: Jia, S. M.. Chinese Academy of Sciences; República de China
Fil: Ge, M. Y.. Chinese Academy of Sciences; República de China
Fil: Liu, Q. Z.. Chinese Academy of Sciences; República de China
Fil: Yan, J. Z.. Chinese Academy of Sciences; República de China
Fil: Li, T. M.. Chinese Academy of Sciences; República de China
Fil: Ren, X. Q.. Chinese Academy of Sciences; República de China
Fil: Ma, R. C.. Chinese Academy of Sciences; República de China
Fil: Zhang, Yuexin. University of Groningen. Departament of Astronomy. Kapteyn Astronómical Institute; Países Bajos
Fil: Zhou, Xudong. Chinese Academy of Sciences; República de China
Fil: Ma, B. Y.. Chinese Academy of Sciences; República de China
Fil: Du, Y. F.. Chinese Academy of Sciences; República de China
Fil: Fu, Y. C.. Chinese Academy of Sciences; República de China
Fil: Xiao, Y. X.. Chinese Academy of Sciences; República de China
Fil: Li, P. P.. Chinese Academy of Sciences; República de China
Fil: Jin, P.. Chinese Academy of Sciences; República de China
Fil: Zhao, S. J.. Chinese Academy of Sciences; República de China
Fil: Zhao, Q. C.. Chinese Academy of Sciences; República de China
Materia: ACCRETION
ACCRETION DISKS
BLACK HOLE PHYSICS
X-RAYS: 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:11336/219009

Acceder

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network_acronym_str	CONICETDig
repository_id_str	3498
network_name_str	CONICET Digital (CONICET)
spelling	Fast transitions of X-ray variability in the black hole transient GX 339−4: comparison with MAXI J1820+070 and MAXI J1348−630Yang, Zi XuZhang, LiangZhang, S. N.Méndez, M.García, FedericoHuang, YueBu, QingcuiLiu, He XinYu, WeiWang, P. J.Tao, L.Altamirano, D.Qu, Jin LuZhang, S.Ma, X.Song, L. M.Jia, S. M.Ge, M. Y.Liu, Q. Z.Yan, J. Z.Li, T. M.Ren, X. Q.Ma, R. C.Zhang, YuexinZhou, XudongMa, B. Y.Du, Y. F.Fu, Y. C.Xiao, Y. X.Li, P. P.Jin, P.Zhao, S. J.Zhao, Q. C.ACCRETIONACCRETION DISKSBLACK HOLE PHYSICSX-RAYS: BINARIEShttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Fast transitions between different types of power density spectra (PDS) happening over time-scales of several tens of seconds are rare phenomena in black hole X-ray binaries. In this paper, we report a broad-band spectral-timing analysis of the fast transitions observed in the 2021 outburst of GX 339-4 using NICER and Insight-HXMT observations. We observe transitions between band-limited noise-dominated PDS and type-B quasi-periodic oscillations (QPOs), and their rapid appearance or disappearance. We also make a detailed comparison between the fast transitions in GX 339-4 with those seen in MAXI J1820+070 and MAXI J1348-630. By comparing the spectra of the periods with and without type-B QPOs, we find that the spectral ratios above 10 keV are nearly constant or slightly decreasing, and the values are different between sources. Below 10 keV, the flux change of the Comptonization component is inversely proportional to the flux change of the thermal component, suggesting that the appearance of type-B QPOs is associated with a redistribution of the accretion power between the disc and the Comptonizing emission region. The spectral ratios between the periods with type-B QPO and those with broad-band noise are significantly different from that with type-B QPO and without type-B QPO, where the ratios (type-B QPO/broad-band noise) show a maximum at around 4 keV and then decrease gradually towards high energies. Finally, we discuss the possible change of the geometry of the inner accretion flow and/or jet during the transitions.Fil: Yang, Zi Xu. Chinese Academy of Sciences; República de ChinaFil: Zhang, Liang. Chinese Academy of Sciences; República de ChinaFil: Zhang, S. N.. Chinese Academy of Sciences; República de ChinaFil: Méndez, M.. Kapteyn Astronomical Institute; Países BajosFil: García, Federico. 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: Huang, Yue. Chinese Academy of Sciences; República de ChinaFil: Bu, Qingcui. Eberhard Karls Universität Tübingen; AlemaniaFil: Liu, He Xin. Chinese Academy of Sciences; República de ChinaFil: Yu, Wei. Chinese Academy of Sciences; República de ChinaFil: Wang, P. J.. Chinese Academy of Sciences; República de ChinaFil: Tao, L.. Chinese Academy of Sciences; República de ChinaFil: Altamirano, D.. University of Southampton; Reino UnidoFil: Qu, Jin Lu. Chinese Academy of Sciences; República de ChinaFil: Zhang, S.. Chinese Academy of Sciences; República de ChinaFil: Ma, X.. Chinese Academy of Sciences; República de ChinaFil: Song, L. M.. Chinese Academy of Sciences; República de ChinaFil: Jia, S. M.. Chinese Academy of Sciences; República de ChinaFil: Ge, M. Y.. Chinese Academy of Sciences; República de ChinaFil: Liu, Q. Z.. Chinese Academy of Sciences; República de ChinaFil: Yan, J. Z.. Chinese Academy of Sciences; República de ChinaFil: Li, T. M.. Chinese Academy of Sciences; República de ChinaFil: Ren, X. Q.. Chinese Academy of Sciences; República de ChinaFil: Ma, R. C.. Chinese Academy of Sciences; República de ChinaFil: Zhang, Yuexin. University of Groningen. Departament of Astronomy. Kapteyn Astronómical Institute; Países BajosFil: Zhou, Xudong. Chinese Academy of Sciences; República de ChinaFil: Ma, B. Y.. Chinese Academy of Sciences; República de ChinaFil: Du, Y. F.. Chinese Academy of Sciences; República de ChinaFil: Fu, Y. C.. Chinese Academy of Sciences; República de ChinaFil: Xiao, Y. X.. Chinese Academy of Sciences; República de ChinaFil: Li, P. P.. Chinese Academy of Sciences; República de ChinaFil: Jin, P.. Chinese Academy of Sciences; República de ChinaFil: Zhao, S. J.. Chinese Academy of Sciences; República de ChinaFil: Zhao, Q. C.. Chinese Academy of Sciences; República de ChinaWiley Blackwell Publishing, Inc2023-05info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/219009Yang, Zi Xu; Zhang, Liang; Zhang, S. N.; Méndez, M.; García, Federico; et al.; Fast transitions of X-ray variability in the black hole transient GX 339−4: comparison with MAXI J1820+070 and MAXI J1348−630; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 521; 3; 5-2023; 3570-35840035-8711CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article/521/3/3570/7080158info:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stad795info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-03T09:47:06Zoai:ri.conicet.gov.ar:11336/219009instacron: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:34982025-09-03 09:47:06.981CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv	Fast transitions of X-ray variability in the black hole transient GX 339−4: comparison with MAXI J1820+070 and MAXI J1348−630
title	Fast transitions of X-ray variability in the black hole transient GX 339−4: comparison with MAXI J1820+070 and MAXI J1348−630
spellingShingle	Fast transitions of X-ray variability in the black hole transient GX 339−4: comparison with MAXI J1820+070 and MAXI J1348−630 Yang, Zi Xu ACCRETION ACCRETION DISKS BLACK HOLE PHYSICS X-RAYS: BINARIES
title_short	Fast transitions of X-ray variability in the black hole transient GX 339−4: comparison with MAXI J1820+070 and MAXI J1348−630
title_full	Fast transitions of X-ray variability in the black hole transient GX 339−4: comparison with MAXI J1820+070 and MAXI J1348−630
title_fullStr	Fast transitions of X-ray variability in the black hole transient GX 339−4: comparison with MAXI J1820+070 and MAXI J1348−630
title_full_unstemmed	Fast transitions of X-ray variability in the black hole transient GX 339−4: comparison with MAXI J1820+070 and MAXI J1348−630
title_sort	Fast transitions of X-ray variability in the black hole transient GX 339−4: comparison with MAXI J1820+070 and MAXI J1348−630
dc.creator.none.fl_str_mv	Yang, Zi Xu Zhang, Liang Zhang, S. N. Méndez, M. García, Federico Huang, Yue Bu, Qingcui Liu, He Xin Yu, Wei Wang, P. J. Tao, L. Altamirano, D. Qu, Jin Lu Zhang, S. Ma, X. Song, L. M. Jia, S. M. Ge, M. Y. Liu, Q. Z. Yan, J. Z. Li, T. M. Ren, X. Q. Ma, R. C. Zhang, Yuexin Zhou, Xudong Ma, B. Y. Du, Y. F. Fu, Y. C. Xiao, Y. X. Li, P. P. Jin, P. Zhao, S. J. Zhao, Q. C.
author	Yang, Zi Xu
author_facet	Yang, Zi Xu Zhang, Liang Zhang, S. N. Méndez, M. García, Federico Huang, Yue Bu, Qingcui Liu, He Xin Yu, Wei Wang, P. J. Tao, L. Altamirano, D. Qu, Jin Lu Zhang, S. Ma, X. Song, L. M. Jia, S. M. Ge, M. Y. Liu, Q. Z. Yan, J. Z. Li, T. M. Ren, X. Q. Ma, R. C. Zhang, Yuexin Zhou, Xudong Ma, B. Y. Du, Y. F. Fu, Y. C. Xiao, Y. X. Li, P. P. Jin, P. Zhao, S. J. Zhao, Q. C.
author_role	author
author2	Zhang, Liang Zhang, S. N. Méndez, M. García, Federico Huang, Yue Bu, Qingcui Liu, He Xin Yu, Wei Wang, P. J. Tao, L. Altamirano, D. Qu, Jin Lu Zhang, S. Ma, X. Song, L. M. Jia, S. M. Ge, M. Y. Liu, Q. Z. Yan, J. Z. Li, T. M. Ren, X. Q. Ma, R. C. Zhang, Yuexin Zhou, Xudong Ma, B. Y. Du, Y. F. Fu, Y. C. Xiao, Y. X. Li, P. P. Jin, P. Zhao, S. J. Zhao, Q. C.
author2_role	author author author author author author author author author author author author 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	ACCRETION ACCRETION DISKS BLACK HOLE PHYSICS X-RAYS: BINARIES
topic	ACCRETION ACCRETION DISKS BLACK HOLE PHYSICS X-RAYS: 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	Fast transitions between different types of power density spectra (PDS) happening over time-scales of several tens of seconds are rare phenomena in black hole X-ray binaries. In this paper, we report a broad-band spectral-timing analysis of the fast transitions observed in the 2021 outburst of GX 339-4 using NICER and Insight-HXMT observations. We observe transitions between band-limited noise-dominated PDS and type-B quasi-periodic oscillations (QPOs), and their rapid appearance or disappearance. We also make a detailed comparison between the fast transitions in GX 339-4 with those seen in MAXI J1820+070 and MAXI J1348-630. By comparing the spectra of the periods with and without type-B QPOs, we find that the spectral ratios above 10 keV are nearly constant or slightly decreasing, and the values are different between sources. Below 10 keV, the flux change of the Comptonization component is inversely proportional to the flux change of the thermal component, suggesting that the appearance of type-B QPOs is associated with a redistribution of the accretion power between the disc and the Comptonizing emission region. The spectral ratios between the periods with type-B QPO and those with broad-band noise are significantly different from that with type-B QPO and without type-B QPO, where the ratios (type-B QPO/broad-band noise) show a maximum at around 4 keV and then decrease gradually towards high energies. Finally, we discuss the possible change of the geometry of the inner accretion flow and/or jet during the transitions. Fil: Yang, Zi Xu. Chinese Academy of Sciences; República de China Fil: Zhang, Liang. Chinese Academy of Sciences; República de China Fil: Zhang, S. N.. Chinese Academy of Sciences; República de China Fil: Méndez, M.. Kapteyn Astronomical Institute; Países Bajos Fil: García, Federico. 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: Huang, Yue. Chinese Academy of Sciences; República de China Fil: Bu, Qingcui. Eberhard Karls Universität Tübingen; Alemania Fil: Liu, He Xin. Chinese Academy of Sciences; República de China Fil: Yu, Wei. Chinese Academy of Sciences; República de China Fil: Wang, P. J.. Chinese Academy of Sciences; República de China Fil: Tao, L.. Chinese Academy of Sciences; República de China Fil: Altamirano, D.. University of Southampton; Reino Unido Fil: Qu, Jin Lu. Chinese Academy of Sciences; República de China Fil: Zhang, S.. Chinese Academy of Sciences; República de China Fil: Ma, X.. Chinese Academy of Sciences; República de China Fil: Song, L. M.. Chinese Academy of Sciences; República de China Fil: Jia, S. M.. Chinese Academy of Sciences; República de China Fil: Ge, M. Y.. Chinese Academy of Sciences; República de China Fil: Liu, Q. Z.. Chinese Academy of Sciences; República de China Fil: Yan, J. Z.. Chinese Academy of Sciences; República de China Fil: Li, T. M.. Chinese Academy of Sciences; República de China Fil: Ren, X. Q.. Chinese Academy of Sciences; República de China Fil: Ma, R. C.. Chinese Academy of Sciences; República de China Fil: Zhang, Yuexin. University of Groningen. Departament of Astronomy. Kapteyn Astronómical Institute; Países Bajos Fil: Zhou, Xudong. Chinese Academy of Sciences; República de China Fil: Ma, B. Y.. Chinese Academy of Sciences; República de China Fil: Du, Y. F.. Chinese Academy of Sciences; República de China Fil: Fu, Y. C.. Chinese Academy of Sciences; República de China Fil: Xiao, Y. X.. Chinese Academy of Sciences; República de China Fil: Li, P. P.. Chinese Academy of Sciences; República de China Fil: Jin, P.. Chinese Academy of Sciences; República de China Fil: Zhao, S. J.. Chinese Academy of Sciences; República de China Fil: Zhao, Q. C.. Chinese Academy of Sciences; República de China
description	Fast transitions between different types of power density spectra (PDS) happening over time-scales of several tens of seconds are rare phenomena in black hole X-ray binaries. In this paper, we report a broad-band spectral-timing analysis of the fast transitions observed in the 2021 outburst of GX 339-4 using NICER and Insight-HXMT observations. We observe transitions between band-limited noise-dominated PDS and type-B quasi-periodic oscillations (QPOs), and their rapid appearance or disappearance. We also make a detailed comparison between the fast transitions in GX 339-4 with those seen in MAXI J1820+070 and MAXI J1348-630. By comparing the spectra of the periods with and without type-B QPOs, we find that the spectral ratios above 10 keV are nearly constant or slightly decreasing, and the values are different between sources. Below 10 keV, the flux change of the Comptonization component is inversely proportional to the flux change of the thermal component, suggesting that the appearance of type-B QPOs is associated with a redistribution of the accretion power between the disc and the Comptonizing emission region. The spectral ratios between the periods with type-B QPO and those with broad-band noise are significantly different from that with type-B QPO and without type-B QPO, where the ratios (type-B QPO/broad-band noise) show a maximum at around 4 keV and then decrease gradually towards high energies. Finally, we discuss the possible change of the geometry of the inner accretion flow and/or jet during the transitions.
publishDate	2023
dc.date.none.fl_str_mv	2023-05
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/11336/219009 Yang, Zi Xu; Zhang, Liang; Zhang, S. N.; Méndez, M.; García, Federico; et al.; Fast transitions of X-ray variability in the black hole transient GX 339−4: comparison with MAXI J1820+070 and MAXI J1348−630; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 521; 3; 5-2023; 3570-3584 0035-8711 CONICET Digital CONICET
url	http://hdl.handle.net/11336/219009
identifier_str_mv	Yang, Zi Xu; Zhang, Liang; Zhang, S. N.; Méndez, M.; García, Federico; et al.; Fast transitions of X-ray variability in the black hole transient GX 339−4: comparison with MAXI J1820+070 and MAXI J1348−630; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 521; 3; 5-2023; 3570-3584 0035-8711 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://academic.oup.com/mnras/article/521/3/3570/7080158 info:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stad795
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	Wiley Blackwell Publishing, Inc
publisher.none.fl_str_mv	Wiley Blackwell Publishing, Inc
dc.source.none.fl_str_mv	reponame:CONICET Digital (CONICET) instname:Consejo Nacional de Investigaciones Científicas y Técnicas
reponame_str	CONICET Digital (CONICET)
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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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Fast transitions of X-ray variability in the black hole transient GX 339−4: comparison with MAXI J1820+070 and MAXI J1348−630

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