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
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/158855
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CONICET Digital (CONICET) |
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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 |
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CONICET Digital (CONICET) |
collection |
CONICET Digital (CONICET) |
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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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1844613652366229504 |
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13.070432 |