On the nature of the hard X-ray source IGR J2018+4043
- Autores
- Bykov, A. M.; Krassilchtchikov, A. M.; Uvarov, Yu. A.; Kennea, J. A.; Pavlov, G. G.; Dubner, Gloria Mabel; Giacani, Elsa Beatriz
- Año de publicación
- 2006
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- We found a very likely counterpart to the recently discovered hard X-ray source IGR J2018 4043 in the multiwavelength observations of the source field. The source, originally discovered in the 20–40 keV band, is now confidently detected also in the 40–80 keV band, with a flux of . A 5 ks 11 2 1 (1.4 0.4) # 10 ergs cm s Swift observation of the IGR J2018 4043 field revealed a hard pointlike source with an observed 0.5–10 keV flux of ergs cm2 s 1 (90% confidence level) at , (with a 4 .2 0.7 12 hms 3.40.8 # 10 a p 20 18 38.55 d p 4041 00 .4 uncertainty). The combined Swift-INTEGRAL spectrum can be described by an absorbed power-law model with photon index and cm2 . In archival optical and infrared data we found a slightly 3.2 22 G p 1.3 0.2 NH p 6.12.2 # 10 extended and highly absorbed object at the Swift source position. There is also an extended VLA 1.4 GHz source peaked at a beamwidth distance from the optical and X-ray positions. The observed morphology and multiwavelength spectra of IGR J2018 4043 are consistent with those expected for an obscured accreting object, i.e., an AGN or a Galactic X-ray binary. The identification suggests possible connection of IGR J2018 4043 to the bright g-ray source GEV J2020 4023 detected by COS B and CGRO EGRET.
Fil: Bykov, A. M.. Russian Academy of Sciences; Rusia
Fil: Krassilchtchikov, A. M.. Russian Academy of Sciences; Rusia
Fil: Uvarov, Yu. A.. Russian Academy of Sciences; Rusia
Fil: Kennea, J. A.. State University of Pennsylvania; Estados Unidos
Fil: Pavlov, G. G.. University of Pennsylvania; Estados Unidos
Fil: Dubner, Gloria Mabel. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina
Fil: Giacani, Elsa Beatriz. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina - Materia
- x-ray
- 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:11336/22172
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On the nature of the hard X-ray source IGR J2018+4043Bykov, A. M.Krassilchtchikov, A. M.Uvarov, Yu. A.Kennea, J. A.Pavlov, G. G.Dubner, Gloria MabelGiacani, Elsa Beatrizx-rayhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We found a very likely counterpart to the recently discovered hard X-ray source IGR J2018 4043 in the multiwavelength observations of the source field. The source, originally discovered in the 20–40 keV band, is now confidently detected also in the 40–80 keV band, with a flux of . A 5 ks 11 2 1 (1.4 0.4) # 10 ergs cm s Swift observation of the IGR J2018 4043 field revealed a hard pointlike source with an observed 0.5–10 keV flux of ergs cm2 s 1 (90% confidence level) at , (with a 4 .2 0.7 12 hms 3.40.8 # 10 a p 20 18 38.55 d p 4041 00 .4 uncertainty). The combined Swift-INTEGRAL spectrum can be described by an absorbed power-law model with photon index and cm2 . In archival optical and infrared data we found a slightly 3.2 22 G p 1.3 0.2 NH p 6.12.2 # 10 extended and highly absorbed object at the Swift source position. There is also an extended VLA 1.4 GHz source peaked at a beamwidth distance from the optical and X-ray positions. The observed morphology and multiwavelength spectra of IGR J2018 4043 are consistent with those expected for an obscured accreting object, i.e., an AGN or a Galactic X-ray binary. The identification suggests possible connection of IGR J2018 4043 to the bright g-ray source GEV J2020 4023 detected by COS B and CGRO EGRET.Fil: Bykov, A. M.. Russian Academy of Sciences; RusiaFil: Krassilchtchikov, A. M.. Russian Academy of Sciences; RusiaFil: Uvarov, Yu. A.. Russian Academy of Sciences; RusiaFil: Kennea, J. A.. State University of Pennsylvania; Estados UnidosFil: Pavlov, G. G.. University of Pennsylvania; Estados UnidosFil: Dubner, Gloria Mabel. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; ArgentinaFil: Giacani, Elsa Beatriz. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; ArgentinaIOP Publishing2006-12info: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/11336/22172Bykov, A. M.; Krassilchtchikov, A. M.; Uvarov, Yu. A.; Kennea, J. A.; Pavlov, G. G.; et al.; On the nature of the hard X-ray source IGR J2018+4043; IOP Publishing; Astrophysical Journal; 649; 1; 12-2006; L21-L240004-637XCONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.1086/508327info:eu-repo/semantics/altIdentifier/doi/10.1086/508327info:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/astro-ph/0609676info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:36:34Zoai:ri.conicet.gov.ar:11336/22172instacron: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 09:36:34.51CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
On the nature of the hard X-ray source IGR J2018+4043 |
title |
On the nature of the hard X-ray source IGR J2018+4043 |
spellingShingle |
On the nature of the hard X-ray source IGR J2018+4043 Bykov, A. M. x-ray |
title_short |
On the nature of the hard X-ray source IGR J2018+4043 |
title_full |
On the nature of the hard X-ray source IGR J2018+4043 |
title_fullStr |
On the nature of the hard X-ray source IGR J2018+4043 |
title_full_unstemmed |
On the nature of the hard X-ray source IGR J2018+4043 |
title_sort |
On the nature of the hard X-ray source IGR J2018+4043 |
dc.creator.none.fl_str_mv |
Bykov, A. M. Krassilchtchikov, A. M. Uvarov, Yu. A. Kennea, J. A. Pavlov, G. G. Dubner, Gloria Mabel Giacani, Elsa Beatriz |
author |
Bykov, A. M. |
author_facet |
Bykov, A. M. Krassilchtchikov, A. M. Uvarov, Yu. A. Kennea, J. A. Pavlov, G. G. Dubner, Gloria Mabel Giacani, Elsa Beatriz |
author_role |
author |
author2 |
Krassilchtchikov, A. M. Uvarov, Yu. A. Kennea, J. A. Pavlov, G. G. Dubner, Gloria Mabel Giacani, Elsa Beatriz |
author2_role |
author author author author author author |
dc.subject.none.fl_str_mv |
x-ray |
topic |
x-ray |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
We found a very likely counterpart to the recently discovered hard X-ray source IGR J2018 4043 in the multiwavelength observations of the source field. The source, originally discovered in the 20–40 keV band, is now confidently detected also in the 40–80 keV band, with a flux of . A 5 ks 11 2 1 (1.4 0.4) # 10 ergs cm s Swift observation of the IGR J2018 4043 field revealed a hard pointlike source with an observed 0.5–10 keV flux of ergs cm2 s 1 (90% confidence level) at , (with a 4 .2 0.7 12 hms 3.40.8 # 10 a p 20 18 38.55 d p 4041 00 .4 uncertainty). The combined Swift-INTEGRAL spectrum can be described by an absorbed power-law model with photon index and cm2 . In archival optical and infrared data we found a slightly 3.2 22 G p 1.3 0.2 NH p 6.12.2 # 10 extended and highly absorbed object at the Swift source position. There is also an extended VLA 1.4 GHz source peaked at a beamwidth distance from the optical and X-ray positions. The observed morphology and multiwavelength spectra of IGR J2018 4043 are consistent with those expected for an obscured accreting object, i.e., an AGN or a Galactic X-ray binary. The identification suggests possible connection of IGR J2018 4043 to the bright g-ray source GEV J2020 4023 detected by COS B and CGRO EGRET. Fil: Bykov, A. M.. Russian Academy of Sciences; Rusia Fil: Krassilchtchikov, A. M.. Russian Academy of Sciences; Rusia Fil: Uvarov, Yu. A.. Russian Academy of Sciences; Rusia Fil: Kennea, J. A.. State University of Pennsylvania; Estados Unidos Fil: Pavlov, G. G.. University of Pennsylvania; Estados Unidos Fil: Dubner, Gloria Mabel. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina Fil: Giacani, Elsa Beatriz. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina |
description |
We found a very likely counterpart to the recently discovered hard X-ray source IGR J2018 4043 in the multiwavelength observations of the source field. The source, originally discovered in the 20–40 keV band, is now confidently detected also in the 40–80 keV band, with a flux of . A 5 ks 11 2 1 (1.4 0.4) # 10 ergs cm s Swift observation of the IGR J2018 4043 field revealed a hard pointlike source with an observed 0.5–10 keV flux of ergs cm2 s 1 (90% confidence level) at , (with a 4 .2 0.7 12 hms 3.40.8 # 10 a p 20 18 38.55 d p 4041 00 .4 uncertainty). The combined Swift-INTEGRAL spectrum can be described by an absorbed power-law model with photon index and cm2 . In archival optical and infrared data we found a slightly 3.2 22 G p 1.3 0.2 NH p 6.12.2 # 10 extended and highly absorbed object at the Swift source position. There is also an extended VLA 1.4 GHz source peaked at a beamwidth distance from the optical and X-ray positions. The observed morphology and multiwavelength spectra of IGR J2018 4043 are consistent with those expected for an obscured accreting object, i.e., an AGN or a Galactic X-ray binary. The identification suggests possible connection of IGR J2018 4043 to the bright g-ray source GEV J2020 4023 detected by COS B and CGRO EGRET. |
publishDate |
2006 |
dc.date.none.fl_str_mv |
2006-12 |
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/11336/22172 Bykov, A. M.; Krassilchtchikov, A. M.; Uvarov, Yu. A.; Kennea, J. A.; Pavlov, G. G.; et al.; On the nature of the hard X-ray source IGR J2018+4043; IOP Publishing; Astrophysical Journal; 649; 1; 12-2006; L21-L24 0004-637X CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/22172 |
identifier_str_mv |
Bykov, A. M.; Krassilchtchikov, A. M.; Uvarov, Yu. A.; Kennea, J. A.; Pavlov, G. G.; et al.; On the nature of the hard X-ray source IGR J2018+4043; IOP Publishing; Astrophysical Journal; 649; 1; 12-2006; L21-L24 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/url/http://iopscience.iop.org/article/10.1086/508327 info:eu-repo/semantics/altIdentifier/doi/10.1086/508327 info:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/astro-ph/0609676 |
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 application/pdf |
dc.publisher.none.fl_str_mv |
IOP Publishing |
publisher.none.fl_str_mv |
IOP Publishing |
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reponame:CONICET Digital (CONICET) instname:Consejo Nacional de Investigaciones Científicas y Técnicas |
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CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas |
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dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar |
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