Microquasar Models for 3EG J1828+0142 and 3EG J1735-1500

Autores
Bosch Ramon, Valentí; Paredes, J. M.; Romero, Gustavo Esteban; Torres, Diego F.
Año de publicación
2005
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
Microquasars are promising candidates to emit high-energy gamma-rays. Moreover, statistical studies show that variable EGRET sources at low galactic latitudes could be associated with the inner spiral arms. The variable nature and the location in the Galaxy of the high-mass microquasars, concentrated in the galactic plane and within 55 degrees from the galactic center, give to these objects the status of likely counterparts of the variable low-latitude EGRET sources. We consider in this work the two most variable EGRET sources at low-latitudes: 3EG J1828+0142 and 3EG J1735-1500, proposing a microquasar model to explain the EGRET data in consistency with the observations at lower energies (from radio frequencies to soft gamma-rays) within the EGRET error box.
Instituto Argentino de Radioastronomía
Facultad de Ciencias Astronómicas y Geofísicas
Materia
Ciencias Astronómicas
X-rays: binaries
Stars: winds, outflows
gamma-rays: observations
gamma-rays: theory
Nivel de accesibilidad
acceso abierto
Condiciones de uso
http://creativecommons.org/licenses/by-nc-sa/4.0/
Repositorio
SEDICI (UNLP)
Institución
Universidad Nacional de La Plata
OAI Identificador
oai:sedici.unlp.edu.ar:10915/127087
Acceder
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oai_identifier_str oai:sedici.unlp.edu.ar:10915/127087
network_acronym_str SEDICI
repository_id_str 1329
network_name_str SEDICI (UNLP)
spelling Microquasar Models for 3EG J1828+0142 and 3EG J1735-1500Bosch Ramon, ValentíParedes, J. M.Romero, Gustavo EstebanTorres, Diego F.Ciencias AstronómicasX-rays: binariesStars: winds, outflowsgamma-rays: observationsgamma-rays: theoryMicroquasars are promising candidates to emit high-energy gamma-rays. Moreover, statistical studies show that variable EGRET sources at low galactic latitudes could be associated with the inner spiral arms. The variable nature and the location in the Galaxy of the high-mass microquasars, concentrated in the galactic plane and within 55 degrees from the galactic center, give to these objects the status of likely counterparts of the variable low-latitude EGRET sources. We consider in this work the two most variable EGRET sources at low-latitudes: 3EG J1828+0142 and 3EG J1735-1500, proposing a microquasar model to explain the EGRET data in consistency with the observations at lower energies (from radio frequencies to soft gamma-rays) within the EGRET error box.Instituto Argentino de RadioastronomíaFacultad de Ciencias Astronómicas y Geofísicas2005-12-31info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdf284-288http://sedici.unlp.edu.ar/handle/10915/127087enginfo:eu-repo/semantics/altIdentifier/issn/1009-9271info:eu-repo/semantics/altIdentifier/doi/10.1088/1009-9271/5/s1/284info:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by-nc-sa/4.0/Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-10-15T11:22:31Zoai:sedici.unlp.edu.ar:10915/127087Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-10-15 11:22:31.805SEDICI (UNLP) - Universidad Nacional de La Platafalse
dc.title.none.fl_str_mv Microquasar Models for 3EG J1828+0142 and 3EG J1735-1500
title Microquasar Models for 3EG J1828+0142 and 3EG J1735-1500
spellingShingle Microquasar Models for 3EG J1828+0142 and 3EG J1735-1500
Bosch Ramon, Valentí
Ciencias Astronómicas
X-rays: binaries
Stars: winds, outflows
gamma-rays: observations
gamma-rays: theory
title_short Microquasar Models for 3EG J1828+0142 and 3EG J1735-1500
title_full Microquasar Models for 3EG J1828+0142 and 3EG J1735-1500
title_fullStr Microquasar Models for 3EG J1828+0142 and 3EG J1735-1500
title_full_unstemmed Microquasar Models for 3EG J1828+0142 and 3EG J1735-1500
title_sort Microquasar Models for 3EG J1828+0142 and 3EG J1735-1500
dc.creator.none.fl_str_mv Bosch Ramon, Valentí
Paredes, J. M.
Romero, Gustavo Esteban
Torres, Diego F.
author Bosch Ramon, Valentí
author_facet Bosch Ramon, Valentí
Paredes, J. M.
Romero, Gustavo Esteban
Torres, Diego F.
author_role author
author2 Paredes, J. M.
Romero, Gustavo Esteban
Torres, Diego F.
author2_role author
author
author
dc.subject.none.fl_str_mv Ciencias Astronómicas
X-rays: binaries
Stars: winds, outflows
gamma-rays: observations
gamma-rays: theory
topic Ciencias Astronómicas
X-rays: binaries
Stars: winds, outflows
gamma-rays: observations
gamma-rays: theory
dc.description.none.fl_txt_mv Microquasars are promising candidates to emit high-energy gamma-rays. Moreover, statistical studies show that variable EGRET sources at low galactic latitudes could be associated with the inner spiral arms. The variable nature and the location in the Galaxy of the high-mass microquasars, concentrated in the galactic plane and within 55 degrees from the galactic center, give to these objects the status of likely counterparts of the variable low-latitude EGRET sources. We consider in this work the two most variable EGRET sources at low-latitudes: 3EG J1828+0142 and 3EG J1735-1500, proposing a microquasar model to explain the EGRET data in consistency with the observations at lower energies (from radio frequencies to soft gamma-rays) within the EGRET error box.
Instituto Argentino de Radioastronomía
Facultad de Ciencias Astronómicas y Geofísicas
description Microquasars are promising candidates to emit high-energy gamma-rays. Moreover, statistical studies show that variable EGRET sources at low galactic latitudes could be associated with the inner spiral arms. The variable nature and the location in the Galaxy of the high-mass microquasars, concentrated in the galactic plane and within 55 degrees from the galactic center, give to these objects the status of likely counterparts of the variable low-latitude EGRET sources. We consider in this work the two most variable EGRET sources at low-latitudes: 3EG J1828+0142 and 3EG J1735-1500, proposing a microquasar model to explain the EGRET data in consistency with the observations at lower energies (from radio frequencies to soft gamma-rays) within the EGRET error box.
publishDate 2005
dc.date.none.fl_str_mv 2005-12-31
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
Articulo
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://sedici.unlp.edu.ar/handle/10915/127087
url http://sedici.unlp.edu.ar/handle/10915/127087
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/issn/1009-9271
info:eu-repo/semantics/altIdentifier/doi/10.1088/1009-9271/5/s1/284
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
http://creativecommons.org/licenses/by-nc-sa/4.0/
Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
eu_rights_str_mv openAccess
rights_invalid_str_mv http://creativecommons.org/licenses/by-nc-sa/4.0/
Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
dc.format.none.fl_str_mv application/pdf
284-288
dc.source.none.fl_str_mv reponame:SEDICI (UNLP)
instname:Universidad Nacional de La Plata
instacron:UNLP
reponame_str SEDICI (UNLP)
collection SEDICI (UNLP)
instname_str Universidad Nacional de La Plata
instacron_str UNLP
institution UNLP
repository.name.fl_str_mv SEDICI (UNLP) - Universidad Nacional de La Plata
repository.mail.fl_str_mv alira@sedici.unlp.edu.ar
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score 13.22299

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