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
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/217983
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oai:ri.conicet.gov.ar:11336/217983 |
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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 Técnicas2025-09-29T10:23:33Zoai: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:34982025-09-29 10:23:33.835CONICET 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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1844614230697836544 |
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13.070432 |