An evolutionary model for the gamma-ray system psr j1311-3430 and its companion

Autores
Benvenuto, Omar Gustavo; De Vito, María Alejandra; Horvath, Jorge Ernesto
Año de publicación
2013
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
The most recent member of the millisecond pulsar with very low mass companions and short orbital periods class, PSR J1311−3430 (Pletsch et al. 2012) is a remarkable object in various senses. Besides being the first discovered in gamma rays, its measured features include the very low or absent hydrogen content. We show in this Letter that this important piece of information leads to a very restricted range of initial periods for a given donor mass. For that purpose, we calculate in detail the evolution of the binary system self-consistently, including mass transfer and evaporation, finding the features of the new evolutionary path leading to the observed configuration. It is also important to remark that the detailed evolutionary history of the system naturally leads to a high final pulsar mass, as it seems to be demanded by observations.
Fil: Benvenuto, Omar Gustavo. Universidad Nacional de la Plata. Facultad de Cs.astronomicas y Geofisicas; Argentina. 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
Fil: De Vito, María Alejandra. 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
Fil: Horvath, Jorge Ernesto. Universidade do Sao Paulo. Instituto Astronomia, Geofisica e Ciencias Atmosfericas; Brasil
Materia
3430
BINARIES: CLOSE
PULSARS: GENERAL
PULSARS: INDIVIDUAL: PSR J1311
STARS: EVOLUTION
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:11336/20508
Acceder
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oai_identifier_str oai:ri.conicet.gov.ar:11336/20508
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repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling An evolutionary model for the gamma-ray system psr j1311-3430 and its companionBenvenuto, Omar GustavoDe Vito, María AlejandraHorvath, Jorge Ernesto3430BINARIES: CLOSEPULSARS: GENERALPULSARS: INDIVIDUAL: PSR J1311STARS: EVOLUTIONhttps://purl.org/becyt/ford/1.7https://purl.org/becyt/ford/1The most recent member of the millisecond pulsar with very low mass companions and short orbital periods class, PSR J1311−3430 (Pletsch et al. 2012) is a remarkable object in various senses. Besides being the first discovered in gamma rays, its measured features include the very low or absent hydrogen content. We show in this Letter that this important piece of information leads to a very restricted range of initial periods for a given donor mass. For that purpose, we calculate in detail the evolution of the binary system self-consistently, including mass transfer and evaporation, finding the features of the new evolutionary path leading to the observed configuration. It is also important to remark that the detailed evolutionary history of the system naturally leads to a high final pulsar mass, as it seems to be demanded by observations.Fil: Benvenuto, Omar Gustavo. Universidad Nacional de la Plata. Facultad de Cs.astronomicas y Geofisicas; Argentina. 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; ArgentinaFil: De Vito, María Alejandra. 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; ArgentinaFil: Horvath, Jorge Ernesto. Universidade do Sao Paulo. Instituto Astronomia, Geofisica e Ciencias Atmosfericas; BrasilWiley-blackwell Publishing, Inc2013-06info: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/11336/20508Benvenuto, Omar Gustavo; De Vito, María Alejandra; Horvath, Jorge Ernesto; An evolutionary model for the gamma-ray system psr j1311-3430 and its companion; Wiley-blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society: Letters; 433; 1; 6-2013; L11-L140035-87111745-3933enginfo:eu-repo/semantics/altIdentifier/url/http://mnrasl.oxfordjournals.org/content/early/2013/05/10/mnrasl.slt046info:eu-repo/semantics/altIdentifier/doi/10.1093/mnrasl/slt046info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-03T09:50:04Zoai:ri.conicet.gov.ar:11336/20508instacron: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:34982025-09-03 09:50:04.342CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv An evolutionary model for the gamma-ray system psr j1311-3430 and its companion
title An evolutionary model for the gamma-ray system psr j1311-3430 and its companion
spellingShingle An evolutionary model for the gamma-ray system psr j1311-3430 and its companion
Benvenuto, Omar Gustavo
3430
BINARIES: CLOSE
PULSARS: GENERAL
PULSARS: INDIVIDUAL: PSR J1311
STARS: EVOLUTION
title_short An evolutionary model for the gamma-ray system psr j1311-3430 and its companion
title_full An evolutionary model for the gamma-ray system psr j1311-3430 and its companion
title_fullStr An evolutionary model for the gamma-ray system psr j1311-3430 and its companion
title_full_unstemmed An evolutionary model for the gamma-ray system psr j1311-3430 and its companion
title_sort An evolutionary model for the gamma-ray system psr j1311-3430 and its companion
dc.creator.none.fl_str_mv Benvenuto, Omar Gustavo
De Vito, María Alejandra
Horvath, Jorge Ernesto
author Benvenuto, Omar Gustavo
author_facet Benvenuto, Omar Gustavo
De Vito, María Alejandra
Horvath, Jorge Ernesto
author_role author
author2 De Vito, María Alejandra
Horvath, Jorge Ernesto
author2_role author
author
dc.subject.none.fl_str_mv 3430
BINARIES: CLOSE
PULSARS: GENERAL
PULSARS: INDIVIDUAL: PSR J1311
STARS: EVOLUTION
topic 3430
BINARIES: CLOSE
PULSARS: GENERAL
PULSARS: INDIVIDUAL: PSR J1311
STARS: EVOLUTION
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.7
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv The most recent member of the millisecond pulsar with very low mass companions and short orbital periods class, PSR J1311−3430 (Pletsch et al. 2012) is a remarkable object in various senses. Besides being the first discovered in gamma rays, its measured features include the very low or absent hydrogen content. We show in this Letter that this important piece of information leads to a very restricted range of initial periods for a given donor mass. For that purpose, we calculate in detail the evolution of the binary system self-consistently, including mass transfer and evaporation, finding the features of the new evolutionary path leading to the observed configuration. It is also important to remark that the detailed evolutionary history of the system naturally leads to a high final pulsar mass, as it seems to be demanded by observations.
Fil: Benvenuto, Omar Gustavo. Universidad Nacional de la Plata. Facultad de Cs.astronomicas y Geofisicas; Argentina. 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
Fil: De Vito, María Alejandra. 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
Fil: Horvath, Jorge Ernesto. Universidade do Sao Paulo. Instituto Astronomia, Geofisica e Ciencias Atmosfericas; Brasil
description The most recent member of the millisecond pulsar with very low mass companions and short orbital periods class, PSR J1311−3430 (Pletsch et al. 2012) is a remarkable object in various senses. Besides being the first discovered in gamma rays, its measured features include the very low or absent hydrogen content. We show in this Letter that this important piece of information leads to a very restricted range of initial periods for a given donor mass. For that purpose, we calculate in detail the evolution of the binary system self-consistently, including mass transfer and evaporation, finding the features of the new evolutionary path leading to the observed configuration. It is also important to remark that the detailed evolutionary history of the system naturally leads to a high final pulsar mass, as it seems to be demanded by observations.
publishDate 2013
dc.date.none.fl_str_mv 2013-06
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/11336/20508
Benvenuto, Omar Gustavo; De Vito, María Alejandra; Horvath, Jorge Ernesto; An evolutionary model for the gamma-ray system psr j1311-3430 and its companion; Wiley-blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society: Letters; 433; 1; 6-2013; L11-L14
0035-8711
1745-3933
url http://hdl.handle.net/11336/20508
identifier_str_mv Benvenuto, Omar Gustavo; De Vito, María Alejandra; Horvath, Jorge Ernesto; An evolutionary model for the gamma-ray system psr j1311-3430 and its companion; Wiley-blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society: Letters; 433; 1; 6-2013; L11-L14
0035-8711
1745-3933
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/url/http://mnrasl.oxfordjournals.org/content/early/2013/05/10/mnrasl.slt046
info:eu-repo/semantics/altIdentifier/doi/10.1093/mnrasl/slt046
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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score 13.13397

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