Microquasar models for 3EG J1828+0142 and 3EG J1735-1500
- Autores
- Bosch Ramon, Valentí; Paredes, Josep Maria; 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.
Fil: Bosch Ramon, Valentí. Universidad de Barcelona; España
Fil: Paredes, Josep Maria. Universidad de Barcelona; España
Fil: Romero, Gustavo Esteban. 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: Torres, Diego F.. Lawrence Livermore National Laboratory; Estados Unidos - Materia
-
Microquasars
Gamma rays - 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:11336/29698
Ver los metadatos del registro completo
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Microquasar models for 3EG J1828+0142 and 3EG J1735-1500Bosch Ramon, ValentíParedes, Josep MariaRomero, Gustavo EstebanTorres, Diego F.MicroquasarsGamma rayshttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Microquasars 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.Fil: Bosch Ramon, Valentí. Universidad de Barcelona; EspañaFil: Paredes, Josep Maria. Universidad de Barcelona; EspañaFil: Romero, Gustavo Esteban. 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: Torres, Diego F.. Lawrence Livermore National Laboratory; Estados UnidosScience Press2005-12info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/29698Bosch Ramon, Valentí; Paredes, Josep Maria; Romero, Gustavo Esteban; Torres, Diego F.; Microquasar models for 3EG J1828+0142 and 3EG J1735-1500; Science Press; Chinese Journal of Astronomy and Astrophysics; 5; 12-2005; 284-2881009-9271CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/http://adsabs.harvard.edu/abs/2005ChJAS...5..284Binfo:eu-repo/semantics/altIdentifier/url/http://articles.adsabs.harvard.edu/full/2005ChJAS...5..284Binfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:45:55Zoai:ri.conicet.gov.ar:11336/29698instacron: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 09:45:55.595CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
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 Microquasars Gamma rays |
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, Josep Maria Romero, Gustavo Esteban Torres, Diego F. |
author |
Bosch Ramon, Valentí |
author_facet |
Bosch Ramon, Valentí Paredes, Josep Maria Romero, Gustavo Esteban Torres, Diego F. |
author_role |
author |
author2 |
Paredes, Josep Maria Romero, Gustavo Esteban Torres, Diego F. |
author2_role |
author author author |
dc.subject.none.fl_str_mv |
Microquasars Gamma rays |
topic |
Microquasars Gamma rays |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
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. Fil: Bosch Ramon, Valentí. Universidad de Barcelona; España Fil: Paredes, Josep Maria. Universidad de Barcelona; España Fil: Romero, Gustavo Esteban. 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: Torres, Diego F.. Lawrence Livermore National Laboratory; Estados Unidos |
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 |
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/11336/29698 Bosch Ramon, Valentí; Paredes, Josep Maria; Romero, Gustavo Esteban; Torres, Diego F.; Microquasar models for 3EG J1828+0142 and 3EG J1735-1500; Science Press; Chinese Journal of Astronomy and Astrophysics; 5; 12-2005; 284-288 1009-9271 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/29698 |
identifier_str_mv |
Bosch Ramon, Valentí; Paredes, Josep Maria; Romero, Gustavo Esteban; Torres, Diego F.; Microquasar models for 3EG J1828+0142 and 3EG J1735-1500; Science Press; Chinese Journal of Astronomy and Astrophysics; 5; 12-2005; 284-288 1009-9271 CONICET Digital CONICET |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/url/http://adsabs.harvard.edu/abs/2005ChJAS...5..284B info:eu-repo/semantics/altIdentifier/url/http://articles.adsabs.harvard.edu/full/2005ChJAS...5..284B |
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 |
Science Press |
publisher.none.fl_str_mv |
Science 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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13.070432 |