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
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/142296
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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 Técnicas2025-09-29T09:46:08Zoai: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:34982025-09-29 09:46:08.662CONICET 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 |
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CONICET Digital (CONICET) |
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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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13.070432 |