Failed-transition outbursts in black hole low-mass X-ray binaries

Autores
Alabarta, K.; Altamirano, D.; Méndez, M.; Cúneo, V. A.; Vincentelli, F. M.; Castro Segura, N.; García, Federico; Luff, B.; Veledina, A.
Año de publicación
2021
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
Black hole low-mass X-ray binaries (BH LMXBs) evolve in a similar way during outburst. Based on the X-ray spectrum and variability, this evolution can be divided into three canonical states: low/hard, intermediate, and high/soft state. BH LMXBs evolve from the low/hard to the high/soft state through the intermediate state in some outbursts (here called ´full outbursts´). However, in other cases, BH LMXBs undergo outbursts in which the source never reaches the high/soft state, here called ´failed-transition outbursts´ (FT outbursts). From a sample of 56 BH LMXBs undergoing 128 outbursts, we find that 36 per cent of these BH LMXBs experienced at least one FT outburst, and that FT outbursts represent ∼33 per cent of the outbursts of the sample, showing that these are common events. We compare all the available X-ray data of full and FT outbursts of BH LMXBs from RXTE/PCA, Swift/BAT, and MAXI, and find that FT and full outbursts cannot be distinguished from their X-ray light curves, hardness-intensity diagrams, or X-ray variability during the initial 10-60 d after the outburst onset. This suggests that both types of outbursts are driven by the same physical process. We also compare the optical and infrared (O/IR) data of FT and full outbursts of GX 339-4. We found that this system is generally brighter in O/IR bands before an FT outburst, suggesting that the O/IR flux points to the physical process that later leads to a full or an FT outburst. We discuss our results in the context of models that describe the onset and evolution of outbursts in accreting X-ray binaries.
Fil: Alabarta, K.. University of Southampton; Reino Unido
Fil: Altamirano, D.. University of Southampton; Reino Unido
Fil: Méndez, M.. University of Groningen; Países Bajos
Fil: Cúneo, V. A.. Universidad de La Laguna; España
Fil: Vincentelli, F. M.. University of Southampton; Reino Unido
Fil: Castro Segura, N.. University of Southampton; Reino Unido
Fil: García, Federico. University of Groningen; Países Bajos
Fil: Luff, B.. University of Southampton; Reino Unido
Fil: Veledina, A.. Royal Institute of Technology; Suecia. University of Turku; Finlandia
Materia
ACCRETION, ACCRETION DISCS
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
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/158855

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network_acronym_str CONICETDig
repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling Failed-transition outbursts in black hole low-mass X-ray binariesAlabarta, K.Altamirano, D.Méndez, M.Cúneo, V. A.Vincentelli, F. M.Castro Segura, N.García, FedericoLuff, B.Veledina, A.ACCRETION, ACCRETION DISCSBLACK HOLE PHYSICSX-RAYS: BINARIEShttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Black hole low-mass X-ray binaries (BH LMXBs) evolve in a similar way during outburst. Based on the X-ray spectrum and variability, this evolution can be divided into three canonical states: low/hard, intermediate, and high/soft state. BH LMXBs evolve from the low/hard to the high/soft state through the intermediate state in some outbursts (here called ´full outbursts´). However, in other cases, BH LMXBs undergo outbursts in which the source never reaches the high/soft state, here called ´failed-transition outbursts´ (FT outbursts). From a sample of 56 BH LMXBs undergoing 128 outbursts, we find that 36 per cent of these BH LMXBs experienced at least one FT outburst, and that FT outbursts represent ∼33 per cent of the outbursts of the sample, showing that these are common events. We compare all the available X-ray data of full and FT outbursts of BH LMXBs from RXTE/PCA, Swift/BAT, and MAXI, and find that FT and full outbursts cannot be distinguished from their X-ray light curves, hardness-intensity diagrams, or X-ray variability during the initial 10-60 d after the outburst onset. This suggests that both types of outbursts are driven by the same physical process. We also compare the optical and infrared (O/IR) data of FT and full outbursts of GX 339-4. We found that this system is generally brighter in O/IR bands before an FT outburst, suggesting that the O/IR flux points to the physical process that later leads to a full or an FT outburst. We discuss our results in the context of models that describe the onset and evolution of outbursts in accreting X-ray binaries.Fil: Alabarta, K.. University of Southampton; Reino UnidoFil: Altamirano, D.. University of Southampton; Reino UnidoFil: Méndez, M.. University of Groningen; Países BajosFil: Cúneo, V. A.. Universidad de La Laguna; EspañaFil: Vincentelli, F. M.. University of Southampton; Reino UnidoFil: Castro Segura, N.. University of Southampton; Reino UnidoFil: García, Federico. University of Groningen; Países BajosFil: Luff, B.. University of Southampton; Reino UnidoFil: Veledina, A.. Royal Institute of Technology; Suecia. University of Turku; FinlandiaWiley Blackwell Publishing, Inc2021-11info: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/11336/158855Alabarta, K.; Altamirano, D.; Méndez, M.; Cúneo, V. A.; Vincentelli, F. M.; et al.; Failed-transition outbursts in black hole low-mass X-ray binaries; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 507; 4; 11-2021; 5507-55220035-8711CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stab2241info:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article/507/4/5507/6352347info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:54:21Zoai:ri.conicet.gov.ar:11336/158855instacron: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:34982025-09-29 09:54:22.139CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Failed-transition outbursts in black hole low-mass X-ray binaries
title Failed-transition outbursts in black hole low-mass X-ray binaries
spellingShingle Failed-transition outbursts in black hole low-mass X-ray binaries
Alabarta, K.
ACCRETION, ACCRETION DISCS
BLACK HOLE PHYSICS
X-RAYS: BINARIES
title_short Failed-transition outbursts in black hole low-mass X-ray binaries
title_full Failed-transition outbursts in black hole low-mass X-ray binaries
title_fullStr Failed-transition outbursts in black hole low-mass X-ray binaries
title_full_unstemmed Failed-transition outbursts in black hole low-mass X-ray binaries
title_sort Failed-transition outbursts in black hole low-mass X-ray binaries
dc.creator.none.fl_str_mv Alabarta, K.
Altamirano, D.
Méndez, M.
Cúneo, V. A.
Vincentelli, F. M.
Castro Segura, N.
García, Federico
Luff, B.
Veledina, A.
author Alabarta, K.
author_facet Alabarta, K.
Altamirano, D.
Méndez, M.
Cúneo, V. A.
Vincentelli, F. M.
Castro Segura, N.
García, Federico
Luff, B.
Veledina, A.
author_role author
author2 Altamirano, D.
Méndez, M.
Cúneo, V. A.
Vincentelli, F. M.
Castro Segura, N.
García, Federico
Luff, B.
Veledina, A.
author2_role author
author
author
author
author
author
author
author
dc.subject.none.fl_str_mv ACCRETION, ACCRETION DISCS
BLACK HOLE PHYSICS
X-RAYS: BINARIES
topic ACCRETION, ACCRETION DISCS
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 Black hole low-mass X-ray binaries (BH LMXBs) evolve in a similar way during outburst. Based on the X-ray spectrum and variability, this evolution can be divided into three canonical states: low/hard, intermediate, and high/soft state. BH LMXBs evolve from the low/hard to the high/soft state through the intermediate state in some outbursts (here called ´full outbursts´). However, in other cases, BH LMXBs undergo outbursts in which the source never reaches the high/soft state, here called ´failed-transition outbursts´ (FT outbursts). From a sample of 56 BH LMXBs undergoing 128 outbursts, we find that 36 per cent of these BH LMXBs experienced at least one FT outburst, and that FT outbursts represent ∼33 per cent of the outbursts of the sample, showing that these are common events. We compare all the available X-ray data of full and FT outbursts of BH LMXBs from RXTE/PCA, Swift/BAT, and MAXI, and find that FT and full outbursts cannot be distinguished from their X-ray light curves, hardness-intensity diagrams, or X-ray variability during the initial 10-60 d after the outburst onset. This suggests that both types of outbursts are driven by the same physical process. We also compare the optical and infrared (O/IR) data of FT and full outbursts of GX 339-4. We found that this system is generally brighter in O/IR bands before an FT outburst, suggesting that the O/IR flux points to the physical process that later leads to a full or an FT outburst. We discuss our results in the context of models that describe the onset and evolution of outbursts in accreting X-ray binaries.
Fil: Alabarta, K.. University of Southampton; Reino Unido
Fil: Altamirano, D.. University of Southampton; Reino Unido
Fil: Méndez, M.. University of Groningen; Países Bajos
Fil: Cúneo, V. A.. Universidad de La Laguna; España
Fil: Vincentelli, F. M.. University of Southampton; Reino Unido
Fil: Castro Segura, N.. University of Southampton; Reino Unido
Fil: García, Federico. University of Groningen; Países Bajos
Fil: Luff, B.. University of Southampton; Reino Unido
Fil: Veledina, A.. Royal Institute of Technology; Suecia. University of Turku; Finlandia
description Black hole low-mass X-ray binaries (BH LMXBs) evolve in a similar way during outburst. Based on the X-ray spectrum and variability, this evolution can be divided into three canonical states: low/hard, intermediate, and high/soft state. BH LMXBs evolve from the low/hard to the high/soft state through the intermediate state in some outbursts (here called ´full outbursts´). However, in other cases, BH LMXBs undergo outbursts in which the source never reaches the high/soft state, here called ´failed-transition outbursts´ (FT outbursts). From a sample of 56 BH LMXBs undergoing 128 outbursts, we find that 36 per cent of these BH LMXBs experienced at least one FT outburst, and that FT outbursts represent ∼33 per cent of the outbursts of the sample, showing that these are common events. We compare all the available X-ray data of full and FT outbursts of BH LMXBs from RXTE/PCA, Swift/BAT, and MAXI, and find that FT and full outbursts cannot be distinguished from their X-ray light curves, hardness-intensity diagrams, or X-ray variability during the initial 10-60 d after the outburst onset. This suggests that both types of outbursts are driven by the same physical process. We also compare the optical and infrared (O/IR) data of FT and full outbursts of GX 339-4. We found that this system is generally brighter in O/IR bands before an FT outburst, suggesting that the O/IR flux points to the physical process that later leads to a full or an FT outburst. We discuss our results in the context of models that describe the onset and evolution of outbursts in accreting X-ray binaries.
publishDate 2021
dc.date.none.fl_str_mv 2021-11
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/11336/158855
Alabarta, K.; Altamirano, D.; Méndez, M.; Cúneo, V. A.; Vincentelli, F. M.; et al.; Failed-transition outbursts in black hole low-mass X-ray binaries; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 507; 4; 11-2021; 5507-5522
0035-8711
CONICET Digital
CONICET
url http://hdl.handle.net/11336/158855
identifier_str_mv Alabarta, K.; Altamirano, D.; Méndez, M.; Cúneo, V. A.; Vincentelli, F. M.; et al.; Failed-transition outbursts in black hole low-mass X-ray binaries; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 507; 4; 11-2021; 5507-5522
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/doi/10.1093/mnras/stab2241
info:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article/507/4/5507/6352347
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 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)
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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