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dc.contributor.author
Bykov, A. M.
dc.contributor.author
Krassilchtchikov, A. M.
dc.contributor.author
Uvarov, Yu. A.
dc.contributor.author
Kennea, J. A.
dc.contributor.author
Pavlov, G. G.
dc.contributor.author
Dubner, Gloria Mabel
dc.contributor.author
Giacani, Elsa Beatriz
dc.date.available
2017-08-11T15:34:00Z
dc.date.issued
2006-12
dc.identifier.citation
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
dc.identifier.issn
0004-637X
dc.identifier.uri
http://hdl.handle.net/11336/22172
dc.description.abstract
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.
dc.format
application/pdf
dc.language.iso
eng
dc.publisher
IOP Publishing
dc.rights
info:eu-repo/semantics/openAccess
dc.rights.uri
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.subject
X-Ray
dc.subject.classification
Astronomía
dc.subject.classification
Ciencias Físicas
dc.subject.classification
CIENCIAS NATURALES Y EXACTAS
dc.title
On the nature of the hard X-ray source IGR J2018+4043
dc.type
info:eu-repo/semantics/article
dc.type
info:ar-repo/semantics/artículo
dc.type
info:eu-repo/semantics/publishedVersion
dc.date.updated
2017-08-07T19:06:32Z
dc.journal.volume
649
dc.journal.number
1
dc.journal.pagination
L21-L24
dc.journal.pais
Reino Unido
dc.journal.ciudad
Londres
dc.description.fil
Fil: Bykov, A. M.. Russian Academy of Sciences; Rusia
dc.description.fil
Fil: Krassilchtchikov, A. M.. Russian Academy of Sciences; Rusia
dc.description.fil
Fil: Uvarov, Yu. A.. Russian Academy of Sciences; Rusia
dc.description.fil
Fil: Kennea, J. A.. State University of Pennsylvania; Estados Unidos
dc.description.fil
Fil: Pavlov, G. G.. University of Pennsylvania; Estados Unidos
dc.description.fil
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
dc.description.fil
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
dc.journal.title
Astrophysical Journal
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.1086/508327
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1086/508327
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/astro-ph/0609676
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