A NuSTAR view of SS433: precessional evolution of the jet-disk system

Autores
Fogantini, Federico Adrián; García, Federico; Combi, Jorge Ariel; Chaty, S.; Martí, Josep; Luque Escamilla, Pedro L.
Año de publicación
2023
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
Context. SS433 is a Galactic microquasar with powerful outflows (double jet, accretion disk and winds) with a well-known orbital, precessional, and nutational period. Aims. In this work we characterise different outflow parameters throughout the precessional cycle of the system. Methods. We analysed ten NuSTAR (3-70 keV) observations of 30 ks that span 1.5 precessional cycles. We extracted averaged spectra and modelled them using a combination of a double thermal jet model (bjet) and pure neutral and relativistic reflection (xillverCp and relxilllpCp) over an accretion disk. Results. We find an average jet bulk velocity of β=v/c0.29 with an opening angle of ²6 deg. Eastern jet kinetic power ranges from 1 to 1039 erg s 1, with base temperatures To ranging from between 14 and 18 keV. Nickel-to-iron abundances remain constant at 9 (within 1I). The western to eastern jet-flux ratio becomes 1 on intermediate phases, which is about 35% of the total precessional orbit. The 3-70 keV total unabsorbed luminosity of the jet and disk ranges from 2 to 20 Ã - 1037 erg s 1, with the disk reflection component mainly contributing to the hard 20-30 keV excess and the stationary 6.7 keV ionised Fe line complex. Conclusions. At low opening angles Î , we find that the jet expands sideways following an adiabatic expansion of a gas with temperature To. Finally, the central source and lower parts of the jet could be hidden by an optically thick region of I >0.1 and size RNH/ne01.5 Ã - 109cm1700rg for MBH=3M-.
Fil: Fogantini, Federico Adrián. 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: 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: Combi, Jorge Ariel. 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: Chaty, S.. Université Paris Cité, CNRS, AstroParticule et Cosmologie; Francia
Fil: Martí, Josep. Universidad de Jaén; España
Fil: Luque Escamilla, Pedro L.. Universidad de Jaén, Campus Las Lagunillas; España
Materia
STARS: JETS
STARS: WINDS, OUTFLOWS
X-RAYS: BINARIES
X-RAYS: INDIVIDUALS: SS433
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:11336/217983
Acceder
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oai_identifier_str oai:ri.conicet.gov.ar:11336/217983
network_acronym_str CONICETDig
repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling A NuSTAR view of SS433: precessional evolution of the jet-disk systemFogantini, Federico AdriánGarcía, FedericoCombi, Jorge ArielChaty, S.Martí, JosepLuque Escamilla, Pedro L.STARS: JETSSTARS: WINDS, OUTFLOWSX-RAYS: BINARIESX-RAYS: INDIVIDUALS: SS433https://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Context. SS433 is a Galactic microquasar with powerful outflows (double jet, accretion disk and winds) with a well-known orbital, precessional, and nutational period. Aims. In this work we characterise different outflow parameters throughout the precessional cycle of the system. Methods. We analysed ten NuSTAR (3-70 keV) observations of 30 ks that span 1.5 precessional cycles. We extracted averaged spectra and modelled them using a combination of a double thermal jet model (bjet) and pure neutral and relativistic reflection (xillverCp and relxilllpCp) over an accretion disk. Results. We find an average jet bulk velocity of β=v/c0.29 with an opening angle of ²6 deg. Eastern jet kinetic power ranges from 1 to 1039 erg s 1, with base temperatures To ranging from between 14 and 18 keV. Nickel-to-iron abundances remain constant at 9 (within 1I). The western to eastern jet-flux ratio becomes 1 on intermediate phases, which is about 35% of the total precessional orbit. The 3-70 keV total unabsorbed luminosity of the jet and disk ranges from 2 to 20 Ã - 1037 erg s 1, with the disk reflection component mainly contributing to the hard 20-30 keV excess and the stationary 6.7 keV ionised Fe line complex. Conclusions. At low opening angles Î , we find that the jet expands sideways following an adiabatic expansion of a gas with temperature To. Finally, the central source and lower parts of the jet could be hidden by an optically thick region of I >0.1 and size RNH/ne01.5 Ã - 109cm1700rg for MBH=3M-.Fil: Fogantini, Federico Adrián. 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: 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: Combi, Jorge Ariel. 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: Chaty, S.. Université Paris Cité, CNRS, AstroParticule et Cosmologie; FranciaFil: Martí, Josep. Universidad de Jaén; EspañaFil: Luque Escamilla, Pedro L.. Universidad de Jaén, Campus Las Lagunillas; EspañaEDP Sciences2023-01info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/217983Fogantini, Federico Adrián; García, Federico; Combi, Jorge Ariel; Chaty, S.; Martí, Josep; et al.; A NuSTAR view of SS433: precessional evolution of the jet-disk system; EDP Sciences; Astronomy and Astrophysics; 669; A149; 1-2023; 1-120004-6361CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361/202243951info:eu-repo/semantics/altIdentifier/url/https://www.aanda.org/articles/aa/full_html/2023/01/aa43951-22/aa43951-22.htmlinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-22T11:56:21Zoai:ri.conicet.gov.ar:11336/217983instacron: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 11:56:22.014CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv A NuSTAR view of SS433: precessional evolution of the jet-disk system
title A NuSTAR view of SS433: precessional evolution of the jet-disk system
spellingShingle A NuSTAR view of SS433: precessional evolution of the jet-disk system
Fogantini, Federico Adrián
STARS: JETS
STARS: WINDS, OUTFLOWS
X-RAYS: BINARIES
X-RAYS: INDIVIDUALS: SS433
title_short A NuSTAR view of SS433: precessional evolution of the jet-disk system
title_full A NuSTAR view of SS433: precessional evolution of the jet-disk system
title_fullStr A NuSTAR view of SS433: precessional evolution of the jet-disk system
title_full_unstemmed A NuSTAR view of SS433: precessional evolution of the jet-disk system
title_sort A NuSTAR view of SS433: precessional evolution of the jet-disk system
dc.creator.none.fl_str_mv Fogantini, Federico Adrián
García, Federico
Combi, Jorge Ariel
Chaty, S.
Martí, Josep
Luque Escamilla, Pedro L.
author Fogantini, Federico Adrián
author_facet Fogantini, Federico Adrián
García, Federico
Combi, Jorge Ariel
Chaty, S.
Martí, Josep
Luque Escamilla, Pedro L.
author_role author
author2 García, Federico
Combi, Jorge Ariel
Chaty, S.
Martí, Josep
Luque Escamilla, Pedro L.
author2_role author
author
author
author
author
dc.subject.none.fl_str_mv STARS: JETS
STARS: WINDS, OUTFLOWS
X-RAYS: BINARIES
X-RAYS: INDIVIDUALS: SS433
topic STARS: JETS
STARS: WINDS, OUTFLOWS
X-RAYS: BINARIES
X-RAYS: INDIVIDUALS: SS433
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv Context. SS433 is a Galactic microquasar with powerful outflows (double jet, accretion disk and winds) with a well-known orbital, precessional, and nutational period. Aims. In this work we characterise different outflow parameters throughout the precessional cycle of the system. Methods. We analysed ten NuSTAR (3-70 keV) observations of 30 ks that span 1.5 precessional cycles. We extracted averaged spectra and modelled them using a combination of a double thermal jet model (bjet) and pure neutral and relativistic reflection (xillverCp and relxilllpCp) over an accretion disk. Results. We find an average jet bulk velocity of β=v/c0.29 with an opening angle of ²6 deg. Eastern jet kinetic power ranges from 1 to 1039 erg s 1, with base temperatures To ranging from between 14 and 18 keV. Nickel-to-iron abundances remain constant at 9 (within 1I). The western to eastern jet-flux ratio becomes 1 on intermediate phases, which is about 35% of the total precessional orbit. The 3-70 keV total unabsorbed luminosity of the jet and disk ranges from 2 to 20 Ã - 1037 erg s 1, with the disk reflection component mainly contributing to the hard 20-30 keV excess and the stationary 6.7 keV ionised Fe line complex. Conclusions. At low opening angles Î , we find that the jet expands sideways following an adiabatic expansion of a gas with temperature To. Finally, the central source and lower parts of the jet could be hidden by an optically thick region of I >0.1 and size RNH/ne01.5 Ã - 109cm1700rg for MBH=3M-.
Fil: Fogantini, Federico Adrián. 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: 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: Combi, Jorge Ariel. 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: Chaty, S.. Université Paris Cité, CNRS, AstroParticule et Cosmologie; Francia
Fil: Martí, Josep. Universidad de Jaén; España
Fil: Luque Escamilla, Pedro L.. Universidad de Jaén, Campus Las Lagunillas; España
description Context. SS433 is a Galactic microquasar with powerful outflows (double jet, accretion disk and winds) with a well-known orbital, precessional, and nutational period. Aims. In this work we characterise different outflow parameters throughout the precessional cycle of the system. Methods. We analysed ten NuSTAR (3-70 keV) observations of 30 ks that span 1.5 precessional cycles. We extracted averaged spectra and modelled them using a combination of a double thermal jet model (bjet) and pure neutral and relativistic reflection (xillverCp and relxilllpCp) over an accretion disk. Results. We find an average jet bulk velocity of β=v/c0.29 with an opening angle of ²6 deg. Eastern jet kinetic power ranges from 1 to 1039 erg s 1, with base temperatures To ranging from between 14 and 18 keV. Nickel-to-iron abundances remain constant at 9 (within 1I). The western to eastern jet-flux ratio becomes 1 on intermediate phases, which is about 35% of the total precessional orbit. The 3-70 keV total unabsorbed luminosity of the jet and disk ranges from 2 to 20 Ã - 1037 erg s 1, with the disk reflection component mainly contributing to the hard 20-30 keV excess and the stationary 6.7 keV ionised Fe line complex. Conclusions. At low opening angles Î , we find that the jet expands sideways following an adiabatic expansion of a gas with temperature To. Finally, the central source and lower parts of the jet could be hidden by an optically thick region of I >0.1 and size RNH/ne01.5 Ã - 109cm1700rg for MBH=3M-.
publishDate 2023
dc.date.none.fl_str_mv 2023-01
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/11336/217983
Fogantini, Federico Adrián; García, Federico; Combi, Jorge Ariel; Chaty, S.; Martí, Josep; et al.; A NuSTAR view of SS433: precessional evolution of the jet-disk system; EDP Sciences; Astronomy and Astrophysics; 669; A149; 1-2023; 1-12
0004-6361
CONICET Digital
CONICET
url http://hdl.handle.net/11336/217983
identifier_str_mv Fogantini, Federico Adrián; García, Federico; Combi, Jorge Ariel; Chaty, S.; Martí, Josep; et al.; A NuSTAR view of SS433: precessional evolution of the jet-disk system; EDP Sciences; Astronomy and Astrophysics; 669; A149; 1-2023; 1-12
0004-6361
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361/202243951
info:eu-repo/semantics/altIdentifier/url/https://www.aanda.org/articles/aa/full_html/2023/01/aa43951-22/aa43951-22.html
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
application/pdf
dc.publisher.none.fl_str_mv EDP Sciences
publisher.none.fl_str_mv EDP Sciences
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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score 12.982451

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