Diagnosing pulsar winds in black-widow, redback, and other binary millisecond pulsar systems

Autores
Zilles, Anne; Kotera, Kumiko; Rohrmann, Rene Daniel; Althaus, Leandro Gabriel
Año de publicación
2020
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
Binary systems composed of a recycled millisecond pulsar and a stellar companion in close orbit could be excellent sites to diagnose pulsar winds. In such systems, the pulsar outflow irradiates and heats up the companion atmosphere, which can lead to the observation of strong day/night modulations in temperature. We demonstrate with particle shower simulations that the particle energy of the wind affects the heating depth in the atmosphere: the wind heat can be deposited above or below the photosphere, leading to different signatures in the observed spectra. We apply our method to four specific systems: We find that systems with cool night-side companions showing strong temperature variations can give interesting lower limits on the particle energy in the winds. In particular, if the companion night side of PSR B1957+20 were to be suddenly irradiated, deep heating would only take place if particles with energy >100 TeV were present. Observational evidence of deep heating in this system thus suggests that (i) such particles exist in the pulsar wind and/or (ii) binary evolution non-trivially takes the companion to the observed temperature asymmetry. Besides, the observed temperature difference can be maintained only with particle energies of the order of 100 MeV.
Fil: Zilles, Anne. Institut D'astrophysique de Paris; Francia. Centre National de la Recherche Scientifique; Francia
Fil: Kotera, Kumiko. Institut D'astrophysique de Paris; Francia. Centre National de la Recherche Scientifique; Francia
Fil: Rohrmann, Rene Daniel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan. Instituto de Ciencias Astronómicas, de la Tierra y del Espacio. Universidad Nacional de San Juan. Instituto de Ciencias Astronómicas, de la Tierra y del Espacio; Argentina
Fil: Althaus, Leandro Gabriel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina
Materia
ACCELERATION OF PARTICLES
ASTROPARTICLE PHYSICS
PULSARS: GENERAL
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:11336/142296
Acceder
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network_name_str CONICET Digital (CONICET)
spelling Diagnosing pulsar winds in black-widow, redback, and other binary millisecond pulsar systemsZilles, AnneKotera, KumikoRohrmann, Rene DanielAlthaus, Leandro GabrielACCELERATION OF PARTICLESASTROPARTICLE PHYSICSPULSARS: GENERALhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Binary systems composed of a recycled millisecond pulsar and a stellar companion in close orbit could be excellent sites to diagnose pulsar winds. In such systems, the pulsar outflow irradiates and heats up the companion atmosphere, which can lead to the observation of strong day/night modulations in temperature. We demonstrate with particle shower simulations that the particle energy of the wind affects the heating depth in the atmosphere: the wind heat can be deposited above or below the photosphere, leading to different signatures in the observed spectra. We apply our method to four specific systems: We find that systems with cool night-side companions showing strong temperature variations can give interesting lower limits on the particle energy in the winds. In particular, if the companion night side of PSR B1957+20 were to be suddenly irradiated, deep heating would only take place if particles with energy >100 TeV were present. Observational evidence of deep heating in this system thus suggests that (i) such particles exist in the pulsar wind and/or (ii) binary evolution non-trivially takes the companion to the observed temperature asymmetry. Besides, the observed temperature difference can be maintained only with particle energies of the order of 100 MeV.Fil: Zilles, Anne. Institut D'astrophysique de Paris; Francia. Centre National de la Recherche Scientifique; FranciaFil: Kotera, Kumiko. Institut D'astrophysique de Paris; Francia. Centre National de la Recherche Scientifique; FranciaFil: Rohrmann, Rene Daniel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan. Instituto de Ciencias Astronómicas, de la Tierra y del Espacio. Universidad Nacional de San Juan. Instituto de Ciencias Astronómicas, de la Tierra y del Espacio; ArgentinaFil: Althaus, Leandro Gabriel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; ArgentinaOxford University Press2020-02info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/142296Zilles, Anne; Kotera, Kumiko; Rohrmann, Rene Daniel; Althaus, Leandro Gabriel; Diagnosing pulsar winds in black-widow, redback, and other binary millisecond pulsar systems; Oxford University Press; Monthly Notices of the Royal Astronomical Society; 492; 2; 2-2020; 1579-15930035-8711CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article/492/2/1579/5672638info:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stz3438info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-15T14:39:41Zoai:ri.conicet.gov.ar:11336/142296instacron: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 14:39:41.864CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Diagnosing pulsar winds in black-widow, redback, and other binary millisecond pulsar systems
title Diagnosing pulsar winds in black-widow, redback, and other binary millisecond pulsar systems
spellingShingle Diagnosing pulsar winds in black-widow, redback, and other binary millisecond pulsar systems
Zilles, Anne
ACCELERATION OF PARTICLES
ASTROPARTICLE PHYSICS
PULSARS: GENERAL
title_short Diagnosing pulsar winds in black-widow, redback, and other binary millisecond pulsar systems
title_full Diagnosing pulsar winds in black-widow, redback, and other binary millisecond pulsar systems
title_fullStr Diagnosing pulsar winds in black-widow, redback, and other binary millisecond pulsar systems
title_full_unstemmed Diagnosing pulsar winds in black-widow, redback, and other binary millisecond pulsar systems
title_sort Diagnosing pulsar winds in black-widow, redback, and other binary millisecond pulsar systems
dc.creator.none.fl_str_mv Zilles, Anne
Kotera, Kumiko
Rohrmann, Rene Daniel
Althaus, Leandro Gabriel
author Zilles, Anne
author_facet Zilles, Anne
Kotera, Kumiko
Rohrmann, Rene Daniel
Althaus, Leandro Gabriel
author_role author
author2 Kotera, Kumiko
Rohrmann, Rene Daniel
Althaus, Leandro Gabriel
author2_role author
author
author
dc.subject.none.fl_str_mv ACCELERATION OF PARTICLES
ASTROPARTICLE PHYSICS
PULSARS: GENERAL
topic ACCELERATION OF PARTICLES
ASTROPARTICLE PHYSICS
PULSARS: GENERAL
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv Binary systems composed of a recycled millisecond pulsar and a stellar companion in close orbit could be excellent sites to diagnose pulsar winds. In such systems, the pulsar outflow irradiates and heats up the companion atmosphere, which can lead to the observation of strong day/night modulations in temperature. We demonstrate with particle shower simulations that the particle energy of the wind affects the heating depth in the atmosphere: the wind heat can be deposited above or below the photosphere, leading to different signatures in the observed spectra. We apply our method to four specific systems: We find that systems with cool night-side companions showing strong temperature variations can give interesting lower limits on the particle energy in the winds. In particular, if the companion night side of PSR B1957+20 were to be suddenly irradiated, deep heating would only take place if particles with energy >100 TeV were present. Observational evidence of deep heating in this system thus suggests that (i) such particles exist in the pulsar wind and/or (ii) binary evolution non-trivially takes the companion to the observed temperature asymmetry. Besides, the observed temperature difference can be maintained only with particle energies of the order of 100 MeV.
Fil: Zilles, Anne. Institut D'astrophysique de Paris; Francia. Centre National de la Recherche Scientifique; Francia
Fil: Kotera, Kumiko. Institut D'astrophysique de Paris; Francia. Centre National de la Recherche Scientifique; Francia
Fil: Rohrmann, Rene Daniel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan. Instituto de Ciencias Astronómicas, de la Tierra y del Espacio. Universidad Nacional de San Juan. Instituto de Ciencias Astronómicas, de la Tierra y del Espacio; Argentina
Fil: Althaus, Leandro Gabriel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina
description Binary systems composed of a recycled millisecond pulsar and a stellar companion in close orbit could be excellent sites to diagnose pulsar winds. In such systems, the pulsar outflow irradiates and heats up the companion atmosphere, which can lead to the observation of strong day/night modulations in temperature. We demonstrate with particle shower simulations that the particle energy of the wind affects the heating depth in the atmosphere: the wind heat can be deposited above or below the photosphere, leading to different signatures in the observed spectra. We apply our method to four specific systems: We find that systems with cool night-side companions showing strong temperature variations can give interesting lower limits on the particle energy in the winds. In particular, if the companion night side of PSR B1957+20 were to be suddenly irradiated, deep heating would only take place if particles with energy >100 TeV were present. Observational evidence of deep heating in this system thus suggests that (i) such particles exist in the pulsar wind and/or (ii) binary evolution non-trivially takes the companion to the observed temperature asymmetry. Besides, the observed temperature difference can be maintained only with particle energies of the order of 100 MeV.
publishDate 2020
dc.date.none.fl_str_mv 2020-02
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/11336/142296
Zilles, Anne; Kotera, Kumiko; Rohrmann, Rene Daniel; Althaus, Leandro Gabriel; Diagnosing pulsar winds in black-widow, redback, and other binary millisecond pulsar systems; Oxford University Press; Monthly Notices of the Royal Astronomical Society; 492; 2; 2-2020; 1579-1593
0035-8711
CONICET Digital
CONICET
url http://hdl.handle.net/11336/142296
identifier_str_mv Zilles, Anne; Kotera, Kumiko; Rohrmann, Rene Daniel; Althaus, Leandro Gabriel; Diagnosing pulsar winds in black-widow, redback, and other binary millisecond pulsar systems; Oxford University Press; Monthly Notices of the Royal Astronomical Society; 492; 2; 2-2020; 1579-1593
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/url/https://academic.oup.com/mnras/article/492/2/1579/5672638
info:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stz3438
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
dc.publisher.none.fl_str_mv Oxford University Press
publisher.none.fl_str_mv Oxford University Press
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 13.22299

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