Dissecting the region of 3EG J1837-0423 and HESS J1841-055 with INTEGRAL
- Autores
- Sguera, V.; Romero, Gustavo Esteban; Bazzano, A.; Masseti, N.; Bird, A. J.; Bassani, L.
- Año de publicación
- 2009
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- 3EG J1837-0423 and HESS J1841-055 are two unidentified and peculiar high-energy sources located in the same region of the sky, separated by 1.4 deg. Specifically, 3EG J1837-0423 is a transient MeV object detected by EGRET only once during flaring activity that lasted a few days while HESS J1841-055 is a highly extended TeV source. We attempted to match the high-energy emission from the unidentified sources 3EG J1837-0423 and HESS J1841-055 with X-rays (4-20 keV) and soft gamma-rays (20-100 keV) candidate counterparts detected through deep INTEGRAL observations of the sky region. As a result we propose the SFXT AX J1841.0-0536 as a possible candidate counterpart of 3EG J1837-0423, based on spatial proximity and transient behavior. Alternatively, AX J1841.0-0536 could be responsible for at least a fraction of the entire TeV emission from the extended source HESS J1841-055, based on a striking spatial correlation. In either case, the proposed association is also supported from an energetic standpoint by a theoretical scenario where AX J1841.0-0536 is a low magnetized pulsar which, due to accretion of massive clumps from the supergiant companion donor star, undergoes sporadic changes to transient Atoll-states where a magnetic tower can produce transient jets and as a consequence high-energy emission. In either case (by association with 3EG J1837-0423 or alternatively with HESS J1841-055), AX J1841.0-0536 might be the prototype of a new class of Galactic transient MeV/TeV emitters.
Fil: Sguera, V.. Istituto di astrofisica spaziale di Bologna; Italia
Fil: Romero, Gustavo Esteban. Provincia de Buenos Aires. Gobernación. Comision de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomia; Argentina. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina
Fil: Bazzano, A.. Istituto Nazionale Di Astrofisica; Italia
Fil: Masseti, N.. Istituto di astrofisica spaziale di Bologna; Italia
Fil: Bird, A. J.. School of Physics and Astronomy; Reino Unido
Fil: Bassani, L.. Istituto Nazionale di Astrofisica; Italia - Materia
-
Gamma ray observations
X ray binaries
X 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:11336/23304
Ver los metadatos del registro completo
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Dissecting the region of 3EG J1837-0423 and HESS J1841-055 with INTEGRALSguera, V.Romero, Gustavo EstebanBazzano, A.Masseti, N.Bird, A. J.Bassani, L.Gamma ray observationsX ray binariesX rayshttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/13EG J1837-0423 and HESS J1841-055 are two unidentified and peculiar high-energy sources located in the same region of the sky, separated by 1.4 deg. Specifically, 3EG J1837-0423 is a transient MeV object detected by EGRET only once during flaring activity that lasted a few days while HESS J1841-055 is a highly extended TeV source. We attempted to match the high-energy emission from the unidentified sources 3EG J1837-0423 and HESS J1841-055 with X-rays (4-20 keV) and soft gamma-rays (20-100 keV) candidate counterparts detected through deep INTEGRAL observations of the sky region. As a result we propose the SFXT AX J1841.0-0536 as a possible candidate counterpart of 3EG J1837-0423, based on spatial proximity and transient behavior. Alternatively, AX J1841.0-0536 could be responsible for at least a fraction of the entire TeV emission from the extended source HESS J1841-055, based on a striking spatial correlation. In either case, the proposed association is also supported from an energetic standpoint by a theoretical scenario where AX J1841.0-0536 is a low magnetized pulsar which, due to accretion of massive clumps from the supergiant companion donor star, undergoes sporadic changes to transient Atoll-states where a magnetic tower can produce transient jets and as a consequence high-energy emission. In either case (by association with 3EG J1837-0423 or alternatively with HESS J1841-055), AX J1841.0-0536 might be the prototype of a new class of Galactic transient MeV/TeV emitters.Fil: Sguera, V.. Istituto di astrofisica spaziale di Bologna; ItaliaFil: Romero, Gustavo Esteban. Provincia de Buenos Aires. Gobernación. Comision de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomia; Argentina. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; ArgentinaFil: Bazzano, A.. Istituto Nazionale Di Astrofisica; ItaliaFil: Masseti, N.. Istituto di astrofisica spaziale di Bologna; ItaliaFil: Bird, A. J.. School of Physics and Astronomy; Reino UnidoFil: Bassani, L.. Istituto Nazionale di Astrofisica; ItaliaIop Publishing2009-12info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/23304Sguera, V.; Romero, Gustavo Esteban; Bazzano, A.; Masseti, N.; Bird, A. J.; et al.; Dissecting the region of 3EG J1837-0423 and HESS J1841-055 with INTEGRAL; Iop Publishing; Astrophysical Journal; 697; 2; 12-2009; 1194-12050004-637XCONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1088/0004-637X/697/2/1194info:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.1088/0004-637X/697/2/1194/metainfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:37:55Zoai:ri.conicet.gov.ar:11336/23304instacron: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 10:37:55.968CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
Dissecting the region of 3EG J1837-0423 and HESS J1841-055 with INTEGRAL |
title |
Dissecting the region of 3EG J1837-0423 and HESS J1841-055 with INTEGRAL |
spellingShingle |
Dissecting the region of 3EG J1837-0423 and HESS J1841-055 with INTEGRAL Sguera, V. Gamma ray observations X ray binaries X rays |
title_short |
Dissecting the region of 3EG J1837-0423 and HESS J1841-055 with INTEGRAL |
title_full |
Dissecting the region of 3EG J1837-0423 and HESS J1841-055 with INTEGRAL |
title_fullStr |
Dissecting the region of 3EG J1837-0423 and HESS J1841-055 with INTEGRAL |
title_full_unstemmed |
Dissecting the region of 3EG J1837-0423 and HESS J1841-055 with INTEGRAL |
title_sort |
Dissecting the region of 3EG J1837-0423 and HESS J1841-055 with INTEGRAL |
dc.creator.none.fl_str_mv |
Sguera, V. Romero, Gustavo Esteban Bazzano, A. Masseti, N. Bird, A. J. Bassani, L. |
author |
Sguera, V. |
author_facet |
Sguera, V. Romero, Gustavo Esteban Bazzano, A. Masseti, N. Bird, A. J. Bassani, L. |
author_role |
author |
author2 |
Romero, Gustavo Esteban Bazzano, A. Masseti, N. Bird, A. J. Bassani, L. |
author2_role |
author author author author author |
dc.subject.none.fl_str_mv |
Gamma ray observations X ray binaries X rays |
topic |
Gamma ray observations X ray binaries X 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 |
3EG J1837-0423 and HESS J1841-055 are two unidentified and peculiar high-energy sources located in the same region of the sky, separated by 1.4 deg. Specifically, 3EG J1837-0423 is a transient MeV object detected by EGRET only once during flaring activity that lasted a few days while HESS J1841-055 is a highly extended TeV source. We attempted to match the high-energy emission from the unidentified sources 3EG J1837-0423 and HESS J1841-055 with X-rays (4-20 keV) and soft gamma-rays (20-100 keV) candidate counterparts detected through deep INTEGRAL observations of the sky region. As a result we propose the SFXT AX J1841.0-0536 as a possible candidate counterpart of 3EG J1837-0423, based on spatial proximity and transient behavior. Alternatively, AX J1841.0-0536 could be responsible for at least a fraction of the entire TeV emission from the extended source HESS J1841-055, based on a striking spatial correlation. In either case, the proposed association is also supported from an energetic standpoint by a theoretical scenario where AX J1841.0-0536 is a low magnetized pulsar which, due to accretion of massive clumps from the supergiant companion donor star, undergoes sporadic changes to transient Atoll-states where a magnetic tower can produce transient jets and as a consequence high-energy emission. In either case (by association with 3EG J1837-0423 or alternatively with HESS J1841-055), AX J1841.0-0536 might be the prototype of a new class of Galactic transient MeV/TeV emitters. Fil: Sguera, V.. Istituto di astrofisica spaziale di Bologna; Italia Fil: Romero, Gustavo Esteban. Provincia de Buenos Aires. Gobernación. Comision de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomia; Argentina. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina Fil: Bazzano, A.. Istituto Nazionale Di Astrofisica; Italia Fil: Masseti, N.. Istituto di astrofisica spaziale di Bologna; Italia Fil: Bird, A. J.. School of Physics and Astronomy; Reino Unido Fil: Bassani, L.. Istituto Nazionale di Astrofisica; Italia |
description |
3EG J1837-0423 and HESS J1841-055 are two unidentified and peculiar high-energy sources located in the same region of the sky, separated by 1.4 deg. Specifically, 3EG J1837-0423 is a transient MeV object detected by EGRET only once during flaring activity that lasted a few days while HESS J1841-055 is a highly extended TeV source. We attempted to match the high-energy emission from the unidentified sources 3EG J1837-0423 and HESS J1841-055 with X-rays (4-20 keV) and soft gamma-rays (20-100 keV) candidate counterparts detected through deep INTEGRAL observations of the sky region. As a result we propose the SFXT AX J1841.0-0536 as a possible candidate counterpart of 3EG J1837-0423, based on spatial proximity and transient behavior. Alternatively, AX J1841.0-0536 could be responsible for at least a fraction of the entire TeV emission from the extended source HESS J1841-055, based on a striking spatial correlation. In either case, the proposed association is also supported from an energetic standpoint by a theoretical scenario where AX J1841.0-0536 is a low magnetized pulsar which, due to accretion of massive clumps from the supergiant companion donor star, undergoes sporadic changes to transient Atoll-states where a magnetic tower can produce transient jets and as a consequence high-energy emission. In either case (by association with 3EG J1837-0423 or alternatively with HESS J1841-055), AX J1841.0-0536 might be the prototype of a new class of Galactic transient MeV/TeV emitters. |
publishDate |
2009 |
dc.date.none.fl_str_mv |
2009-12 |
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/11336/23304 Sguera, V.; Romero, Gustavo Esteban; Bazzano, A.; Masseti, N.; Bird, A. J.; et al.; Dissecting the region of 3EG J1837-0423 and HESS J1841-055 with INTEGRAL; Iop Publishing; Astrophysical Journal; 697; 2; 12-2009; 1194-1205 0004-637X CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/23304 |
identifier_str_mv |
Sguera, V.; Romero, Gustavo Esteban; Bazzano, A.; Masseti, N.; Bird, A. J.; et al.; Dissecting the region of 3EG J1837-0423 and HESS J1841-055 with INTEGRAL; Iop Publishing; Astrophysical Journal; 697; 2; 12-2009; 1194-1205 0004-637X CONICET Digital CONICET |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/doi/10.1088/0004-637X/697/2/1194 info:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.1088/0004-637X/697/2/1194/meta |
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/ |
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application/pdf application/pdf |
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Iop Publishing |
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Iop Publishing |
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CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas |
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