On the peculiar long-term orbital evolution of the eclipsing accreting millisecond X-ray pulsar SWIFT J1749.4 - 2807

Autores
Sanna, A.; Burderi, L.; Salvo, T. Di; Riggio, A.; Altamirano, D.; Marino, A.; Bult, P.; Strohmayer, T. E.; Guillot, S.; Malacaria, C.; Ng, M.; Mancuso, Giulio Cesare; Mazzola, S. M.; Albayati, A. C.; Iaria, R.; Manca, A.; Deiosso, N.; Cabras, C.; Anitra, A.
Año de publicación
2022
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
We present the pulsar timing analysis of the accreting millisecond X-ray pulsar SWIFT J1749.4 - 2807 monitored by NICER and XMM-Newton during its latest outburst after almost 11 yr of quiescence. From the coherent timing analysis of the pulse profiles, we updated the orbital ephemerides of the system. Large phase jumps of the fundamental frequency phase of the signal are visible during the outburst, consistent with what was observed during the previous outburst. Moreover, we report on the marginally significant evidence for non-zero eccentricity (e ≃ 4 × 10-5) obtained independently from the analysis of both the 2021 and 2010 outbursts and we discuss possible compatible scenarios. Long-term orbital evolution of SWIFT J1749.4 - 2807 suggests a fast expansion of both the NS projected semimajor axis (x), and the orbital period (Porb), at a rate of $dot{x}simeq 2.6imes 10^{-13}, ext{lt-s}, ext{s}^{-1}$ and $dot{P}{m orb}simeq 4 imes 10^{-10}, ext{s}, ext{s}^{-1}$, respectively. SWIFT J1749.4 - 2807 is the only accreting millisecond X-ray pulsar, so far, from which the orbital period derivative has been directly measured from appreciable changes on the observed orbital period. Finally, no significant secular deceleration of the spin frequency of the compact object is detected, which allowed us to set a constraint on the magnetic field strength at the polar caps of BPC < 1.3 × 108 G, in line with typical values reported for AMXPs.
Fil: Sanna, A.. Università Degli Studi Di Cagliari; Italia
Fil: Burderi, L.. Università Degli Studi Di Cagliari; Italia
Fil: Salvo, T. Di. Università Degli Studi Di Palermo; Italia
Fil: Riggio, A.. Università Degli Studi Di Cagliari; Italia
Fil: Altamirano, D.. University of Southampton; Reino Unido
Fil: Marino, A.. Instituto de Estudios Espaciales de Cataluña; España
Fil: Bult, P.. University of Maryland; Estados Unidos
Fil: Strohmayer, T. E.. Nasa Goddard Space Flight Center; Estados Unidos
Fil: Guillot, S.. Universite Paul Sabatier Toulouse; Francia
Fil: Malacaria, C.. Huntsville Program Office; Estados Unidos
Fil: Ng, M.. Mit Kavli Institute For Astrophysics And Space Research; Estados Unidos
Fil: Mancuso, Giulio Cesare. 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: Mazzola, S. M.. Università Degli Studi Di Cagliari; Italia
Fil: Albayati, A. C.. University of Southampton; Reino Unido
Fil: Iaria, R.. Università Degli Studi Di Palermo; Italia
Fil: Manca, A.. Università Degli Studi Di Cagliari; Italia
Fil: Deiosso, N.. Università Degli Studi Di Cagliari; Italia
Fil: Cabras, C.. Università Degli Studi Di Cagliari; Italia
Fil: Anitra, A.. Università Degli Studi Di Palermo; Italia
Materia
ACCRETION, ACCRETION DISCS
BINARIES: GENERAL
STARS: NEUTRON
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:11336/203954
Acceder
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network_name_str CONICET Digital (CONICET)
spelling On the peculiar long-term orbital evolution of the eclipsing accreting millisecond X-ray pulsar SWIFT J1749.4 - 2807Sanna, A.Burderi, L.Salvo, T. DiRiggio, A.Altamirano, D.Marino, A.Bult, P.Strohmayer, T. E.Guillot, S.Malacaria, C.Ng, M.Mancuso, Giulio CesareMazzola, S. M.Albayati, A. C.Iaria, R.Manca, A.Deiosso, N.Cabras, C.Anitra, A.ACCRETION, ACCRETION DISCSBINARIES: GENERALSTARS: NEUTRONX-RAYS: BINARIEShttps://purl.org/becyt/ford/1.7https://purl.org/becyt/ford/1We present the pulsar timing analysis of the accreting millisecond X-ray pulsar SWIFT J1749.4 - 2807 monitored by NICER and XMM-Newton during its latest outburst after almost 11 yr of quiescence. From the coherent timing analysis of the pulse profiles, we updated the orbital ephemerides of the system. Large phase jumps of the fundamental frequency phase of the signal are visible during the outburst, consistent with what was observed during the previous outburst. Moreover, we report on the marginally significant evidence for non-zero eccentricity (e ≃ 4 × 10-5) obtained independently from the analysis of both the 2021 and 2010 outbursts and we discuss possible compatible scenarios. Long-term orbital evolution of SWIFT J1749.4 - 2807 suggests a fast expansion of both the NS projected semimajor axis (x), and the orbital period (Porb), at a rate of $dot{x}simeq 2.6imes 10^{-13}, ext{lt-s}, ext{s}^{-1}$ and $dot{P}{m orb}simeq 4 imes 10^{-10}, ext{s}, ext{s}^{-1}$, respectively. SWIFT J1749.4 - 2807 is the only accreting millisecond X-ray pulsar, so far, from which the orbital period derivative has been directly measured from appreciable changes on the observed orbital period. Finally, no significant secular deceleration of the spin frequency of the compact object is detected, which allowed us to set a constraint on the magnetic field strength at the polar caps of BPC < 1.3 × 108 G, in line with typical values reported for AMXPs.Fil: Sanna, A.. Università Degli Studi Di Cagliari; ItaliaFil: Burderi, L.. Università Degli Studi Di Cagliari; ItaliaFil: Salvo, T. Di. Università Degli Studi Di Palermo; ItaliaFil: Riggio, A.. Università Degli Studi Di Cagliari; ItaliaFil: Altamirano, D.. University of Southampton; Reino UnidoFil: Marino, A.. Instituto de Estudios Espaciales de Cataluña; EspañaFil: Bult, P.. University of Maryland; Estados UnidosFil: Strohmayer, T. E.. Nasa Goddard Space Flight Center; Estados UnidosFil: Guillot, S.. Universite Paul Sabatier Toulouse; FranciaFil: Malacaria, C.. Huntsville Program Office; Estados UnidosFil: Ng, M.. Mit Kavli Institute For Astrophysics And Space Research; Estados UnidosFil: Mancuso, Giulio Cesare. 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: Mazzola, S. M.. Università Degli Studi Di Cagliari; ItaliaFil: Albayati, A. C.. University of Southampton; Reino UnidoFil: Iaria, R.. Università Degli Studi Di Palermo; ItaliaFil: Manca, A.. Università Degli Studi Di Cagliari; ItaliaFil: Deiosso, N.. Università Degli Studi Di Cagliari; ItaliaFil: Cabras, C.. Università Degli Studi Di Cagliari; ItaliaFil: Anitra, A.. Università Degli Studi Di Palermo; ItaliaWiley Blackwell Publishing, Inc2022-08info: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/11336/203954Sanna, A.; Burderi, L.; Salvo, T. Di; Riggio, A.; Altamirano, D.; et al.; On the peculiar long-term orbital evolution of the eclipsing accreting millisecond X-ray pulsar SWIFT J1749.4 - 2807; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 514; 3; 8-2022; 4385-43970035-8711CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stac1611info:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article-abstract/514/3/4385/6608272?redirectedFrom=fulltextinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-15T15:29:20Zoai:ri.conicet.gov.ar:11336/203954instacron: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:34982025-10-15 15:29:20.384CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv On the peculiar long-term orbital evolution of the eclipsing accreting millisecond X-ray pulsar SWIFT J1749.4 - 2807
title On the peculiar long-term orbital evolution of the eclipsing accreting millisecond X-ray pulsar SWIFT J1749.4 - 2807
spellingShingle On the peculiar long-term orbital evolution of the eclipsing accreting millisecond X-ray pulsar SWIFT J1749.4 - 2807
Sanna, A.
ACCRETION, ACCRETION DISCS
BINARIES: GENERAL
STARS: NEUTRON
X-RAYS: BINARIES
title_short On the peculiar long-term orbital evolution of the eclipsing accreting millisecond X-ray pulsar SWIFT J1749.4 - 2807
title_full On the peculiar long-term orbital evolution of the eclipsing accreting millisecond X-ray pulsar SWIFT J1749.4 - 2807
title_fullStr On the peculiar long-term orbital evolution of the eclipsing accreting millisecond X-ray pulsar SWIFT J1749.4 - 2807
title_full_unstemmed On the peculiar long-term orbital evolution of the eclipsing accreting millisecond X-ray pulsar SWIFT J1749.4 - 2807
title_sort On the peculiar long-term orbital evolution of the eclipsing accreting millisecond X-ray pulsar SWIFT J1749.4 - 2807
dc.creator.none.fl_str_mv Sanna, A.
Burderi, L.
Salvo, T. Di
Riggio, A.
Altamirano, D.
Marino, A.
Bult, P.
Strohmayer, T. E.
Guillot, S.
Malacaria, C.
Ng, M.
Mancuso, Giulio Cesare
Mazzola, S. M.
Albayati, A. C.
Iaria, R.
Manca, A.
Deiosso, N.
Cabras, C.
Anitra, A.
author Sanna, A.
author_facet Sanna, A.
Burderi, L.
Salvo, T. Di
Riggio, A.
Altamirano, D.
Marino, A.
Bult, P.
Strohmayer, T. E.
Guillot, S.
Malacaria, C.
Ng, M.
Mancuso, Giulio Cesare
Mazzola, S. M.
Albayati, A. C.
Iaria, R.
Manca, A.
Deiosso, N.
Cabras, C.
Anitra, A.
author_role author
author2 Burderi, L.
Salvo, T. Di
Riggio, A.
Altamirano, D.
Marino, A.
Bult, P.
Strohmayer, T. E.
Guillot, S.
Malacaria, C.
Ng, M.
Mancuso, Giulio Cesare
Mazzola, S. M.
Albayati, A. C.
Iaria, R.
Manca, A.
Deiosso, N.
Cabras, C.
Anitra, A.
author2_role 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 DISCS
BINARIES: GENERAL
STARS: NEUTRON
X-RAYS: BINARIES
topic ACCRETION, ACCRETION DISCS
BINARIES: GENERAL
STARS: NEUTRON
X-RAYS: BINARIES
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.7
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv We present the pulsar timing analysis of the accreting millisecond X-ray pulsar SWIFT J1749.4 - 2807 monitored by NICER and XMM-Newton during its latest outburst after almost 11 yr of quiescence. From the coherent timing analysis of the pulse profiles, we updated the orbital ephemerides of the system. Large phase jumps of the fundamental frequency phase of the signal are visible during the outburst, consistent with what was observed during the previous outburst. Moreover, we report on the marginally significant evidence for non-zero eccentricity (e ≃ 4 × 10-5) obtained independently from the analysis of both the 2021 and 2010 outbursts and we discuss possible compatible scenarios. Long-term orbital evolution of SWIFT J1749.4 - 2807 suggests a fast expansion of both the NS projected semimajor axis (x), and the orbital period (Porb), at a rate of $dot{x}simeq 2.6imes 10^{-13}, ext{lt-s}, ext{s}^{-1}$ and $dot{P}{m orb}simeq 4 imes 10^{-10}, ext{s}, ext{s}^{-1}$, respectively. SWIFT J1749.4 - 2807 is the only accreting millisecond X-ray pulsar, so far, from which the orbital period derivative has been directly measured from appreciable changes on the observed orbital period. Finally, no significant secular deceleration of the spin frequency of the compact object is detected, which allowed us to set a constraint on the magnetic field strength at the polar caps of BPC < 1.3 × 108 G, in line with typical values reported for AMXPs.
Fil: Sanna, A.. Università Degli Studi Di Cagliari; Italia
Fil: Burderi, L.. Università Degli Studi Di Cagliari; Italia
Fil: Salvo, T. Di. Università Degli Studi Di Palermo; Italia
Fil: Riggio, A.. Università Degli Studi Di Cagliari; Italia
Fil: Altamirano, D.. University of Southampton; Reino Unido
Fil: Marino, A.. Instituto de Estudios Espaciales de Cataluña; España
Fil: Bult, P.. University of Maryland; Estados Unidos
Fil: Strohmayer, T. E.. Nasa Goddard Space Flight Center; Estados Unidos
Fil: Guillot, S.. Universite Paul Sabatier Toulouse; Francia
Fil: Malacaria, C.. Huntsville Program Office; Estados Unidos
Fil: Ng, M.. Mit Kavli Institute For Astrophysics And Space Research; Estados Unidos
Fil: Mancuso, Giulio Cesare. 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: Mazzola, S. M.. Università Degli Studi Di Cagliari; Italia
Fil: Albayati, A. C.. University of Southampton; Reino Unido
Fil: Iaria, R.. Università Degli Studi Di Palermo; Italia
Fil: Manca, A.. Università Degli Studi Di Cagliari; Italia
Fil: Deiosso, N.. Università Degli Studi Di Cagliari; Italia
Fil: Cabras, C.. Università Degli Studi Di Cagliari; Italia
Fil: Anitra, A.. Università Degli Studi Di Palermo; Italia
description We present the pulsar timing analysis of the accreting millisecond X-ray pulsar SWIFT J1749.4 - 2807 monitored by NICER and XMM-Newton during its latest outburst after almost 11 yr of quiescence. From the coherent timing analysis of the pulse profiles, we updated the orbital ephemerides of the system. Large phase jumps of the fundamental frequency phase of the signal are visible during the outburst, consistent with what was observed during the previous outburst. Moreover, we report on the marginally significant evidence for non-zero eccentricity (e ≃ 4 × 10-5) obtained independently from the analysis of both the 2021 and 2010 outbursts and we discuss possible compatible scenarios. Long-term orbital evolution of SWIFT J1749.4 - 2807 suggests a fast expansion of both the NS projected semimajor axis (x), and the orbital period (Porb), at a rate of $dot{x}simeq 2.6imes 10^{-13}, ext{lt-s}, ext{s}^{-1}$ and $dot{P}{m orb}simeq 4 imes 10^{-10}, ext{s}, ext{s}^{-1}$, respectively. SWIFT J1749.4 - 2807 is the only accreting millisecond X-ray pulsar, so far, from which the orbital period derivative has been directly measured from appreciable changes on the observed orbital period. Finally, no significant secular deceleration of the spin frequency of the compact object is detected, which allowed us to set a constraint on the magnetic field strength at the polar caps of BPC < 1.3 × 108 G, in line with typical values reported for AMXPs.
publishDate 2022
dc.date.none.fl_str_mv 2022-08
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/11336/203954
Sanna, A.; Burderi, L.; Salvo, T. Di; Riggio, A.; Altamirano, D.; et al.; On the peculiar long-term orbital evolution of the eclipsing accreting millisecond X-ray pulsar SWIFT J1749.4 - 2807; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 514; 3; 8-2022; 4385-4397
0035-8711
CONICET Digital
CONICET
url http://hdl.handle.net/11336/203954
identifier_str_mv Sanna, A.; Burderi, L.; Salvo, T. Di; Riggio, A.; Altamirano, D.; et al.; On the peculiar long-term orbital evolution of the eclipsing accreting millisecond X-ray pulsar SWIFT J1749.4 - 2807; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 514; 3; 8-2022; 4385-4397
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/stac1611
info:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article-abstract/514/3/4385/6608272?redirectedFrom=fulltext
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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