TeV J2032+4130: a not-so-dark accelerator?

Autores
Butt, Y. M.; Combi, Jorge Ariel; Drake, J.; Finley, J. P.; Konopelko, A.; Lister, M.; Rodriguez, J.; Shepherd, D.
Año de publicación
2008
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
The HEGRA ã-ray source TeV J2032+4130 is considered the prototypical `dark accelerator´, since it was the first TeV source detected with no firm counterparts at lower frequencies. The Whipple collaboration observed this source in 2003-05 and the emission hotspot appears displaced about 9 arcmin to the northeast of the HEGRA position, though given the large positional uncertainties the HEGRA and Whipple positions are consistent. Here we report on Westerbork Synthesis Radio Telescope (WSRT), Very Large Array (VLA), Chandra and INTEGRAL data covering the locations of the Whipple and HEGRA hotspots. We confirm a dual-lobed radio source coincident with the Whipple hotspot, as well as a weak, partially non-thermal shell-like object, with a location and morphology very similar to the HEGRA source, in our WSRT and mosaicked VLA data sets, respectively. Due to its extended nature, it is likely that the latter structure is a more plausible counterpart of the reported very high-energy (VHE) ã-ray emissions in this region. If so, TeV J2032+4130 may not be a `dark accelerator´ after all. Further observations with the new generation of imaging Cherenkov telescopes are needed to pin down the precise location and morphology of the TeV emission region and thus clear up the confusion over its possible lower frequency counterparts.
Fil: Butt, Y. M.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos
Fil: Combi, Jorge Ariel. 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
Fil: Drake, J.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos
Fil: Finley, J. P.. Purdue University; Estados Unidos
Fil: Konopelko, A.. Purdue University; Estados Unidos
Fil: Lister, M.. Purdue University; Estados Unidos
Fil: Rodriguez, J.. Centre D; Francia
Fil: Shepherd, D.. Purdue University; Estados Unidos
Materia
Acceleration of particles
Magnetic fields
Cosmic rays
Supernova remnants
TeV J2032+4130 (radiofuente)
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/22644

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network_name_str CONICET Digital (CONICET)
spelling TeV J2032+4130: a not-so-dark accelerator?Butt, Y. M.Combi, Jorge ArielDrake, J.Finley, J. P.Konopelko, A.Lister, M.Rodriguez, J.Shepherd, D.Acceleration of particlesMagnetic fieldsCosmic raysSupernova remnantsTeV J2032+4130 (radiofuente)https://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1The HEGRA ã-ray source TeV J2032+4130 is considered the prototypical `dark accelerator´, since it was the first TeV source detected with no firm counterparts at lower frequencies. The Whipple collaboration observed this source in 2003-05 and the emission hotspot appears displaced about 9 arcmin to the northeast of the HEGRA position, though given the large positional uncertainties the HEGRA and Whipple positions are consistent. Here we report on Westerbork Synthesis Radio Telescope (WSRT), Very Large Array (VLA), Chandra and INTEGRAL data covering the locations of the Whipple and HEGRA hotspots. We confirm a dual-lobed radio source coincident with the Whipple hotspot, as well as a weak, partially non-thermal shell-like object, with a location and morphology very similar to the HEGRA source, in our WSRT and mosaicked VLA data sets, respectively. Due to its extended nature, it is likely that the latter structure is a more plausible counterpart of the reported very high-energy (VHE) ã-ray emissions in this region. If so, TeV J2032+4130 may not be a `dark accelerator´ after all. Further observations with the new generation of imaging Cherenkov telescopes are needed to pin down the precise location and morphology of the TeV emission region and thus clear up the confusion over its possible lower frequency counterparts.Fil: Butt, Y. M.. Harvard-Smithsonian Center for Astrophysics; Estados UnidosFil: Combi, Jorge Ariel. 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; ArgentinaFil: Drake, J.. Harvard-Smithsonian Center for Astrophysics; Estados UnidosFil: Finley, J. P.. Purdue University; Estados UnidosFil: Konopelko, A.. Purdue University; Estados UnidosFil: Lister, M.. Purdue University; Estados UnidosFil: Rodriguez, J.. Centre D; FranciaFil: Shepherd, D.. Purdue University; Estados UnidosWiley Blackwell Publishing, Inc2008-12info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/22644Butt, Y. M.; Combi, Jorge Ariel; Drake, J.; Finley, J. P.; Konopelko, A.; et al.; TeV J2032+4130: a not-so-dark accelerator?; Wiley Blackwell Publishing, Inc; Monthly Notices Of The Royal Astronomical Society; 385; 4; 12-2008; 1764-17700035-8711CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/http://onlinelibrary.wiley.com/doi/10.1111/j.1365-2966.2008.12959.x/fullinfo:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article-lookup/doi/10.1111/j.1365-2966.2008.12959.xinfo:eu-repo/semantics/altIdentifier/url/http://dx.doi.org/10.1111/j.1365-2966.2008.12959.xinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:09:25Zoai:ri.conicet.gov.ar:11336/22644instacron: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 10:09:25.923CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv TeV J2032+4130: a not-so-dark accelerator?
title TeV J2032+4130: a not-so-dark accelerator?
spellingShingle TeV J2032+4130: a not-so-dark accelerator?
Butt, Y. M.
Acceleration of particles
Magnetic fields
Cosmic rays
Supernova remnants
TeV J2032+4130 (radiofuente)
title_short TeV J2032+4130: a not-so-dark accelerator?
title_full TeV J2032+4130: a not-so-dark accelerator?
title_fullStr TeV J2032+4130: a not-so-dark accelerator?
title_full_unstemmed TeV J2032+4130: a not-so-dark accelerator?
title_sort TeV J2032+4130: a not-so-dark accelerator?
dc.creator.none.fl_str_mv Butt, Y. M.
Combi, Jorge Ariel
Drake, J.
Finley, J. P.
Konopelko, A.
Lister, M.
Rodriguez, J.
Shepherd, D.
author Butt, Y. M.
author_facet Butt, Y. M.
Combi, Jorge Ariel
Drake, J.
Finley, J. P.
Konopelko, A.
Lister, M.
Rodriguez, J.
Shepherd, D.
author_role author
author2 Combi, Jorge Ariel
Drake, J.
Finley, J. P.
Konopelko, A.
Lister, M.
Rodriguez, J.
Shepherd, D.
author2_role author
author
author
author
author
author
author
dc.subject.none.fl_str_mv Acceleration of particles
Magnetic fields
Cosmic rays
Supernova remnants
TeV J2032+4130 (radiofuente)
topic Acceleration of particles
Magnetic fields
Cosmic rays
Supernova remnants
TeV J2032+4130 (radiofuente)
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv The HEGRA ã-ray source TeV J2032+4130 is considered the prototypical `dark accelerator´, since it was the first TeV source detected with no firm counterparts at lower frequencies. The Whipple collaboration observed this source in 2003-05 and the emission hotspot appears displaced about 9 arcmin to the northeast of the HEGRA position, though given the large positional uncertainties the HEGRA and Whipple positions are consistent. Here we report on Westerbork Synthesis Radio Telescope (WSRT), Very Large Array (VLA), Chandra and INTEGRAL data covering the locations of the Whipple and HEGRA hotspots. We confirm a dual-lobed radio source coincident with the Whipple hotspot, as well as a weak, partially non-thermal shell-like object, with a location and morphology very similar to the HEGRA source, in our WSRT and mosaicked VLA data sets, respectively. Due to its extended nature, it is likely that the latter structure is a more plausible counterpart of the reported very high-energy (VHE) ã-ray emissions in this region. If so, TeV J2032+4130 may not be a `dark accelerator´ after all. Further observations with the new generation of imaging Cherenkov telescopes are needed to pin down the precise location and morphology of the TeV emission region and thus clear up the confusion over its possible lower frequency counterparts.
Fil: Butt, Y. M.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos
Fil: Combi, Jorge Ariel. 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
Fil: Drake, J.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos
Fil: Finley, J. P.. Purdue University; Estados Unidos
Fil: Konopelko, A.. Purdue University; Estados Unidos
Fil: Lister, M.. Purdue University; Estados Unidos
Fil: Rodriguez, J.. Centre D; Francia
Fil: Shepherd, D.. Purdue University; Estados Unidos
description The HEGRA ã-ray source TeV J2032+4130 is considered the prototypical `dark accelerator´, since it was the first TeV source detected with no firm counterparts at lower frequencies. The Whipple collaboration observed this source in 2003-05 and the emission hotspot appears displaced about 9 arcmin to the northeast of the HEGRA position, though given the large positional uncertainties the HEGRA and Whipple positions are consistent. Here we report on Westerbork Synthesis Radio Telescope (WSRT), Very Large Array (VLA), Chandra and INTEGRAL data covering the locations of the Whipple and HEGRA hotspots. We confirm a dual-lobed radio source coincident with the Whipple hotspot, as well as a weak, partially non-thermal shell-like object, with a location and morphology very similar to the HEGRA source, in our WSRT and mosaicked VLA data sets, respectively. Due to its extended nature, it is likely that the latter structure is a more plausible counterpart of the reported very high-energy (VHE) ã-ray emissions in this region. If so, TeV J2032+4130 may not be a `dark accelerator´ after all. Further observations with the new generation of imaging Cherenkov telescopes are needed to pin down the precise location and morphology of the TeV emission region and thus clear up the confusion over its possible lower frequency counterparts.
publishDate 2008
dc.date.none.fl_str_mv 2008-12
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/11336/22644
Butt, Y. M.; Combi, Jorge Ariel; Drake, J.; Finley, J. P.; Konopelko, A.; et al.; TeV J2032+4130: a not-so-dark accelerator?; Wiley Blackwell Publishing, Inc; Monthly Notices Of The Royal Astronomical Society; 385; 4; 12-2008; 1764-1770
0035-8711
CONICET Digital
CONICET
url http://hdl.handle.net/11336/22644
identifier_str_mv Butt, Y. M.; Combi, Jorge Ariel; Drake, J.; Finley, J. P.; Konopelko, A.; et al.; TeV J2032+4130: a not-so-dark accelerator?; Wiley Blackwell Publishing, Inc; Monthly Notices Of The Royal Astronomical Society; 385; 4; 12-2008; 1764-1770
0035-8711
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://onlinelibrary.wiley.com/doi/10.1111/j.1365-2966.2008.12959.x/full
info:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article-lookup/doi/10.1111/j.1365-2966.2008.12959.x
info:eu-repo/semantics/altIdentifier/url/http://dx.doi.org/10.1111/j.1365-2966.2008.12959.x
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 Wiley Blackwell Publishing, Inc
publisher.none.fl_str_mv Wiley Blackwell Publishing, Inc
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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