Unidentified γ-ray sources off the Galactic plane as low-mass microquasars?
- Autores
- Grenier, I. A.; Kaufman Bernadó, María Marina; Romero, Gustavo Esteban
- Año de publicación
- 2005
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- A subset of the unidentified EGRET γ -ray sources with no active galactic nucleus or other conspicuous counterpart appears to be concentrated at medium latitudes. Their long-term variability and their spatial distribution indicate that they are distinct from the more persistent sources associated with the nearby Gould Belt. They exhibit a large scale height of 1.3 ± 0.6 kpc above the Galactic plane. Potential counterparts for these sources include microquasars accreting from a low-mass star and spewing a continuous jet. Detailed calculations have been performed of the jet inverse Compton emission in the radiation fields from the star, the accretion disc, and a hot corona. Different jet Lorentz factors, powers, and aspect angles have been explored. The up-scattered emission from the corona predominates below 100 MeV whereas the disc and stellar contributions are preponderant at higher energies for moderate (∼15◦) and small (∼1◦) aspect angles, respectively. Yet, unlike in the highmass, brighter versions of these systems, the external Compton emission largely fails to produce the luminosities required for 5 to 10 kpc distant EGRET sources. Synchrotron-self-Compton emission appears as a promising alternative.
Fil: Grenier, I. A.. Université Paris VII & Service d’Astrophysique; Francia
Fil: Kaufman Bernadó, María Marina. 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: 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 - Materia
-
X-Ray Binaries
Gamma Ray Observations
Gamma Ray Sources
Unidentified Sources
Microquasars - 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:11336/27798
Ver los metadatos del registro completo
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Unidentified γ-ray sources off the Galactic plane as low-mass microquasars?Grenier, I. A.Kaufman Bernadó, María MarinaRomero, Gustavo EstebanX-Ray BinariesGamma Ray ObservationsGamma Ray SourcesUnidentified SourcesMicroquasarshttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1A subset of the unidentified EGRET γ -ray sources with no active galactic nucleus or other conspicuous counterpart appears to be concentrated at medium latitudes. Their long-term variability and their spatial distribution indicate that they are distinct from the more persistent sources associated with the nearby Gould Belt. They exhibit a large scale height of 1.3 ± 0.6 kpc above the Galactic plane. Potential counterparts for these sources include microquasars accreting from a low-mass star and spewing a continuous jet. Detailed calculations have been performed of the jet inverse Compton emission in the radiation fields from the star, the accretion disc, and a hot corona. Different jet Lorentz factors, powers, and aspect angles have been explored. The up-scattered emission from the corona predominates below 100 MeV whereas the disc and stellar contributions are preponderant at higher energies for moderate (∼15◦) and small (∼1◦) aspect angles, respectively. Yet, unlike in the highmass, brighter versions of these systems, the external Compton emission largely fails to produce the luminosities required for 5 to 10 kpc distant EGRET sources. Synchrotron-self-Compton emission appears as a promising alternative.Fil: Grenier, I. A.. Université Paris VII & Service d’Astrophysique; FranciaFil: Kaufman Bernadó, María Marina. 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: 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; ArgentinaSpringer2005-06info: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/11336/27798Grenier, I. A.; Kaufman Bernadó, María Marina; Romero, Gustavo Esteban; Unidentified γ-ray sources off the Galactic plane as low-mass microquasars?; Springer; Astrophysics And Space Science; 297; 1-4; 6-2005; 109-1180004-640X1572-946XCONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1007/s10509-005-7586-xinfo:eu-repo/semantics/altIdentifier/url/https://link.springer.com/article/10.1007/s10509-005-7586-xinfo:eu-repo/semantics/altIdentifier/arxiv/https://arxiv.org/abs/astro-ph/0408215v1info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:52:44Zoai:ri.conicet.gov.ar:11336/27798instacron: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 09:52:44.962CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
Unidentified γ-ray sources off the Galactic plane as low-mass microquasars? |
title |
Unidentified γ-ray sources off the Galactic plane as low-mass microquasars? |
spellingShingle |
Unidentified γ-ray sources off the Galactic plane as low-mass microquasars? Grenier, I. A. X-Ray Binaries Gamma Ray Observations Gamma Ray Sources Unidentified Sources Microquasars |
title_short |
Unidentified γ-ray sources off the Galactic plane as low-mass microquasars? |
title_full |
Unidentified γ-ray sources off the Galactic plane as low-mass microquasars? |
title_fullStr |
Unidentified γ-ray sources off the Galactic plane as low-mass microquasars? |
title_full_unstemmed |
Unidentified γ-ray sources off the Galactic plane as low-mass microquasars? |
title_sort |
Unidentified γ-ray sources off the Galactic plane as low-mass microquasars? |
dc.creator.none.fl_str_mv |
Grenier, I. A. Kaufman Bernadó, María Marina Romero, Gustavo Esteban |
author |
Grenier, I. A. |
author_facet |
Grenier, I. A. Kaufman Bernadó, María Marina Romero, Gustavo Esteban |
author_role |
author |
author2 |
Kaufman Bernadó, María Marina Romero, Gustavo Esteban |
author2_role |
author author |
dc.subject.none.fl_str_mv |
X-Ray Binaries Gamma Ray Observations Gamma Ray Sources Unidentified Sources Microquasars |
topic |
X-Ray Binaries Gamma Ray Observations Gamma Ray Sources Unidentified Sources Microquasars |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
A subset of the unidentified EGRET γ -ray sources with no active galactic nucleus or other conspicuous counterpart appears to be concentrated at medium latitudes. Their long-term variability and their spatial distribution indicate that they are distinct from the more persistent sources associated with the nearby Gould Belt. They exhibit a large scale height of 1.3 ± 0.6 kpc above the Galactic plane. Potential counterparts for these sources include microquasars accreting from a low-mass star and spewing a continuous jet. Detailed calculations have been performed of the jet inverse Compton emission in the radiation fields from the star, the accretion disc, and a hot corona. Different jet Lorentz factors, powers, and aspect angles have been explored. The up-scattered emission from the corona predominates below 100 MeV whereas the disc and stellar contributions are preponderant at higher energies for moderate (∼15◦) and small (∼1◦) aspect angles, respectively. Yet, unlike in the highmass, brighter versions of these systems, the external Compton emission largely fails to produce the luminosities required for 5 to 10 kpc distant EGRET sources. Synchrotron-self-Compton emission appears as a promising alternative. Fil: Grenier, I. A.. Université Paris VII & Service d’Astrophysique; Francia Fil: Kaufman Bernadó, María Marina. 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: 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 |
description |
A subset of the unidentified EGRET γ -ray sources with no active galactic nucleus or other conspicuous counterpart appears to be concentrated at medium latitudes. Their long-term variability and their spatial distribution indicate that they are distinct from the more persistent sources associated with the nearby Gould Belt. They exhibit a large scale height of 1.3 ± 0.6 kpc above the Galactic plane. Potential counterparts for these sources include microquasars accreting from a low-mass star and spewing a continuous jet. Detailed calculations have been performed of the jet inverse Compton emission in the radiation fields from the star, the accretion disc, and a hot corona. Different jet Lorentz factors, powers, and aspect angles have been explored. The up-scattered emission from the corona predominates below 100 MeV whereas the disc and stellar contributions are preponderant at higher energies for moderate (∼15◦) and small (∼1◦) aspect angles, respectively. Yet, unlike in the highmass, brighter versions of these systems, the external Compton emission largely fails to produce the luminosities required for 5 to 10 kpc distant EGRET sources. Synchrotron-self-Compton emission appears as a promising alternative. |
publishDate |
2005 |
dc.date.none.fl_str_mv |
2005-06 |
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/11336/27798 Grenier, I. A.; Kaufman Bernadó, María Marina; Romero, Gustavo Esteban; Unidentified γ-ray sources off the Galactic plane as low-mass microquasars?; Springer; Astrophysics And Space Science; 297; 1-4; 6-2005; 109-118 0004-640X 1572-946X CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/27798 |
identifier_str_mv |
Grenier, I. A.; Kaufman Bernadó, María Marina; Romero, Gustavo Esteban; Unidentified γ-ray sources off the Galactic plane as low-mass microquasars?; Springer; Astrophysics And Space Science; 297; 1-4; 6-2005; 109-118 0004-640X 1572-946X CONICET Digital CONICET |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/doi/10.1007/s10509-005-7586-x info:eu-repo/semantics/altIdentifier/url/https://link.springer.com/article/10.1007/s10509-005-7586-x info:eu-repo/semantics/altIdentifier/arxiv/https://arxiv.org/abs/astro-ph/0408215v1 |
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 |
Springer |
publisher.none.fl_str_mv |
Springer |
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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1844613616315138048 |
score |
13.070432 |