Deep Morphological and Spectral Study of the SNR RCW 86 with Fermi-LAT

Autores
Ajello, M.; Baldini, L.; Barbiellini, G.; Bastieri, D.; Bellazzini, R.; Bissaldi, E.; Bloom, E. D.; Bonino, R.; Bottacini, E.; Brandt, T. J.; Bregeon, J.; Bruel, P.; Buehler, R.; Caliandro, G. A.; Cameron, R. A.; Caragiulo, M.; Cavazzuti, E.; Charles, E.; Chekhtman, A.; Ciprini, S.; Cohen Tanugi, J.; Condon, E.; Costanza, F.; Cutini, F.; D’Ammando, F.; De Palma, F.; Desiante, R.; Dubner, Gloria Mabel; Duvidovich, Laura Patricia; Giacani, Elsa Beatriz; FERMI-LAT Collaboration
Año de publicación
2016
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
RCW 86 is a young supernova remnant (SNR) showing a shell-type structure at several wavelengths and is thought to be an efficient cosmic-ray (CR) accelerator. Earlier Fermi Large Area Telescope results reported the detection of γ-ray emission coincident with the position of RCW 86 but its origin (leptonic or hadronic) remained unclear due to the poor statistics. Thanks to 6.5 years of data acquired by the Fermi-LAT and the new event reconstruction Pass 8, we report the significant detection of spatially extended emission coming from RCW 86. The spectrum is described by a power-law function with a very hard photon index ({{Γ }}=1.42+/- {0.1}{{stat}}+/- {0.06}{{syst}}) in the 0.1?500 GeV range and an energy flux above 100 MeV of (2.91+/- {0.8}{{stat}}+/- {0.12}{{syst}}) × {10}-11 erg cm‑2 s‑1. Gathering all the available multiwavelength (MWL) data, we perform a broadband modeling of the nonthermal emission of RCW 86 to constrain parameters of the nearby medium and bring new hints about the origin of the γ-ray emission. For the whole SNR, the modeling favors a leptonic scenario in the framework of a two-zone model with an average magnetic field of 10.2 ± 0.7 μG and a limit on the maximum energy injected into protons of 2 × 1049 erg for a density of 1 cm‑3. In addition, parameter values are derived for the north?east and south?west (SW) regions of RCW 86, providing the first indication of a higher magnetic field in the SW region.
Fil: Ajello, M.. Clemson University; Estados Unidos
Fil: Baldini, L.. University Of Stanford; Estados Unidos
Fil: Barbiellini, G.. Universita Degli Studi Di Trieste; Italia
Fil: Bastieri, D.. Universita Di Padova; Italia
Fil: Bellazzini, R.. Istituto Nazionale di Fisica Nucleare; Italia
Fil: Bissaldi, E.. Istituto Nazionale di Fisica Nucleare; Italia
Fil: Bloom, E. D.. University Of Stanford; Estados Unidos
Fil: Bonino, R.. Universita degli Studi di Torino; Italia
Fil: Bottacini, E.. University Of Stanford; Estados Unidos
Fil: Brandt, T. J.. National Aeronautics And Space Administration. Goddart Institute For Space Studies; Estados Unidos
Fil: Bregeon, J.. Universite Montpellier II; Francia
Fil: Bruel, P.. Ecole Polytechnique; Francia
Fil: Buehler, R.. Deutsches Elektronen Synchrotron DESY; Alemania
Fil: Caliandro, G. A.. University Of Stanford; Estados Unidos
Fil: Cameron, R. A.. University Of Stanford; Estados Unidos
Fil: Caragiulo, M.. Universita Degli Studi Di Bari; Italia
Fil: Cavazzuti, E.. Agenzia Spaziale Italiana; Italia
Fil: Charles, E.. University Of Stanford; Estados Unidos
Fil: Chekhtman, A.. George Mason University; Estados Unidos
Fil: Ciprini, S.. Agenzia Spaziale Italiana; Italia
Fil: Cohen Tanugi, J.. Universite Montpellier II; Francia
Fil: Condon, E.. Universit´e Bordeaux; Francia
Fil: Costanza, F.. Istituto Nazionale di Fisica Nucleare; Italia
Fil: Cutini, F.. Osservatorio Astronomico di Roma; Italia
Fil: D’Ammando, F.. Universita Di Bologna; Italia
Fil: De Palma, F.. Universita Telematica Pegaso, Piazza Trieste e Trento; Italia
Fil: Desiante, R.. Universita di Udine; Italia
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: Duvidovich, Laura Patricia. 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
Fil: FERMI-LAT Collaboration.
Materia
ACCELERATION OF PARTICLRS
COSMIC RAYS
ISM:INDIVIDUAL OBJECT:RCW 86
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:11336/18847

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repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling Deep Morphological and Spectral Study of the SNR RCW 86 with Fermi-LATAjello, M.Baldini, L.Barbiellini, G.Bastieri, D.Bellazzini, R.Bissaldi, E.Bloom, E. D.Bonino, R.Bottacini, E.Brandt, T. J.Bregeon, J.Bruel, P.Buehler, R.Caliandro, G. A.Cameron, R. A.Caragiulo, M.Cavazzuti, E.Charles, E.Chekhtman, A.Ciprini, S.Cohen Tanugi, J.Condon, E.Costanza, F.Cutini, F.D’Ammando, F.De Palma, F.Desiante, R.Dubner, Gloria MabelDuvidovich, Laura PatriciaGiacani, Elsa BeatrizFERMI-LAT CollaborationACCELERATION OF PARTICLRSCOSMIC RAYSISM:INDIVIDUAL OBJECT:RCW 86https://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1RCW 86 is a young supernova remnant (SNR) showing a shell-type structure at several wavelengths and is thought to be an efficient cosmic-ray (CR) accelerator. Earlier Fermi Large Area Telescope results reported the detection of γ-ray emission coincident with the position of RCW 86 but its origin (leptonic or hadronic) remained unclear due to the poor statistics. Thanks to 6.5 years of data acquired by the Fermi-LAT and the new event reconstruction Pass 8, we report the significant detection of spatially extended emission coming from RCW 86. The spectrum is described by a power-law function with a very hard photon index ({{Γ }}=1.42+/- {0.1}{{stat}}+/- {0.06}{{syst}}) in the 0.1?500 GeV range and an energy flux above 100 MeV of (2.91+/- {0.8}{{stat}}+/- {0.12}{{syst}}) × {10}-11 erg cm‑2 s‑1. Gathering all the available multiwavelength (MWL) data, we perform a broadband modeling of the nonthermal emission of RCW 86 to constrain parameters of the nearby medium and bring new hints about the origin of the γ-ray emission. For the whole SNR, the modeling favors a leptonic scenario in the framework of a two-zone model with an average magnetic field of 10.2 ± 0.7 μG and a limit on the maximum energy injected into protons of 2 × 1049 erg for a density of 1 cm‑3. In addition, parameter values are derived for the north?east and south?west (SW) regions of RCW 86, providing the first indication of a higher magnetic field in the SW region.Fil: Ajello, M.. Clemson University; Estados UnidosFil: Baldini, L.. University Of Stanford; Estados UnidosFil: Barbiellini, G.. Universita Degli Studi Di Trieste; ItaliaFil: Bastieri, D.. Universita Di Padova; ItaliaFil: Bellazzini, R.. Istituto Nazionale di Fisica Nucleare; ItaliaFil: Bissaldi, E.. Istituto Nazionale di Fisica Nucleare; ItaliaFil: Bloom, E. D.. University Of Stanford; Estados UnidosFil: Bonino, R.. Universita degli Studi di Torino; ItaliaFil: Bottacini, E.. University Of Stanford; Estados UnidosFil: Brandt, T. J.. National Aeronautics And Space Administration. Goddart Institute For Space Studies; Estados UnidosFil: Bregeon, J.. Universite Montpellier II; FranciaFil: Bruel, P.. Ecole Polytechnique; FranciaFil: Buehler, R.. Deutsches Elektronen Synchrotron DESY; AlemaniaFil: Caliandro, G. A.. University Of Stanford; Estados UnidosFil: Cameron, R. A.. University Of Stanford; Estados UnidosFil: Caragiulo, M.. Universita Degli Studi Di Bari; ItaliaFil: Cavazzuti, E.. Agenzia Spaziale Italiana; ItaliaFil: Charles, E.. University Of Stanford; Estados UnidosFil: Chekhtman, A.. George Mason University; Estados UnidosFil: Ciprini, S.. Agenzia Spaziale Italiana; ItaliaFil: Cohen Tanugi, J.. Universite Montpellier II; FranciaFil: Condon, E.. Universit´e Bordeaux; FranciaFil: Costanza, F.. Istituto Nazionale di Fisica Nucleare; ItaliaFil: Cutini, F.. Osservatorio Astronomico di Roma; ItaliaFil: D’Ammando, F.. Universita Di Bologna; ItaliaFil: De Palma, F.. Universita Telematica Pegaso, Piazza Trieste e Trento; ItaliaFil: Desiante, R.. Universita di Udine; ItaliaFil: 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: Duvidovich, Laura Patricia. 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; ArgentinaFil: FERMI-LAT Collaboration.Iop Publishing2016-03info: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/11336/18847Ajello, M.; Baldini, L.; Barbiellini, G.; Bastieri, D.; Bellazzini, R.; et al.; Deep Morphological and Spectral Study of the SNR RCW 86 with Fermi-LAT; Iop Publishing; Astrophysical Journal; 819; 2; 3-2016; 1-130004-637XCONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/1601.06534info:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.3847/0004-637X/819/2/98/metainfo:eu-repo/semantics/altIdentifier/doi/doi:10.3847/0004-637X/819/2/98info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:16:29Zoai:ri.conicet.gov.ar:11336/18847instacron: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 10:16:29.963CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Deep Morphological and Spectral Study of the SNR RCW 86 with Fermi-LAT
title Deep Morphological and Spectral Study of the SNR RCW 86 with Fermi-LAT
spellingShingle Deep Morphological and Spectral Study of the SNR RCW 86 with Fermi-LAT
Ajello, M.
ACCELERATION OF PARTICLRS
COSMIC RAYS
ISM:INDIVIDUAL OBJECT:RCW 86
title_short Deep Morphological and Spectral Study of the SNR RCW 86 with Fermi-LAT
title_full Deep Morphological and Spectral Study of the SNR RCW 86 with Fermi-LAT
title_fullStr Deep Morphological and Spectral Study of the SNR RCW 86 with Fermi-LAT
title_full_unstemmed Deep Morphological and Spectral Study of the SNR RCW 86 with Fermi-LAT
title_sort Deep Morphological and Spectral Study of the SNR RCW 86 with Fermi-LAT
dc.creator.none.fl_str_mv Ajello, M.
Baldini, L.
Barbiellini, G.
Bastieri, D.
Bellazzini, R.
Bissaldi, E.
Bloom, E. D.
Bonino, R.
Bottacini, E.
Brandt, T. J.
Bregeon, J.
Bruel, P.
Buehler, R.
Caliandro, G. A.
Cameron, R. A.
Caragiulo, M.
Cavazzuti, E.
Charles, E.
Chekhtman, A.
Ciprini, S.
Cohen Tanugi, J.
Condon, E.
Costanza, F.
Cutini, F.
D’Ammando, F.
De Palma, F.
Desiante, R.
Dubner, Gloria Mabel
Duvidovich, Laura Patricia
Giacani, Elsa Beatriz
FERMI-LAT Collaboration
author Ajello, M.
author_facet Ajello, M.
Baldini, L.
Barbiellini, G.
Bastieri, D.
Bellazzini, R.
Bissaldi, E.
Bloom, E. D.
Bonino, R.
Bottacini, E.
Brandt, T. J.
Bregeon, J.
Bruel, P.
Buehler, R.
Caliandro, G. A.
Cameron, R. A.
Caragiulo, M.
Cavazzuti, E.
Charles, E.
Chekhtman, A.
Ciprini, S.
Cohen Tanugi, J.
Condon, E.
Costanza, F.
Cutini, F.
D’Ammando, F.
De Palma, F.
Desiante, R.
Dubner, Gloria Mabel
Duvidovich, Laura Patricia
Giacani, Elsa Beatriz
FERMI-LAT Collaboration
author_role author
author2 Baldini, L.
Barbiellini, G.
Bastieri, D.
Bellazzini, R.
Bissaldi, E.
Bloom, E. D.
Bonino, R.
Bottacini, E.
Brandt, T. J.
Bregeon, J.
Bruel, P.
Buehler, R.
Caliandro, G. A.
Cameron, R. A.
Caragiulo, M.
Cavazzuti, E.
Charles, E.
Chekhtman, A.
Ciprini, S.
Cohen Tanugi, J.
Condon, E.
Costanza, F.
Cutini, F.
D’Ammando, F.
De Palma, F.
Desiante, R.
Dubner, Gloria Mabel
Duvidovich, Laura Patricia
Giacani, Elsa Beatriz
FERMI-LAT Collaboration
author2_role author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
dc.subject.none.fl_str_mv ACCELERATION OF PARTICLRS
COSMIC RAYS
ISM:INDIVIDUAL OBJECT:RCW 86
topic ACCELERATION OF PARTICLRS
COSMIC RAYS
ISM:INDIVIDUAL OBJECT:RCW 86
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv RCW 86 is a young supernova remnant (SNR) showing a shell-type structure at several wavelengths and is thought to be an efficient cosmic-ray (CR) accelerator. Earlier Fermi Large Area Telescope results reported the detection of γ-ray emission coincident with the position of RCW 86 but its origin (leptonic or hadronic) remained unclear due to the poor statistics. Thanks to 6.5 years of data acquired by the Fermi-LAT and the new event reconstruction Pass 8, we report the significant detection of spatially extended emission coming from RCW 86. The spectrum is described by a power-law function with a very hard photon index ({{Γ }}=1.42+/- {0.1}{{stat}}+/- {0.06}{{syst}}) in the 0.1?500 GeV range and an energy flux above 100 MeV of (2.91+/- {0.8}{{stat}}+/- {0.12}{{syst}}) × {10}-11 erg cm‑2 s‑1. Gathering all the available multiwavelength (MWL) data, we perform a broadband modeling of the nonthermal emission of RCW 86 to constrain parameters of the nearby medium and bring new hints about the origin of the γ-ray emission. For the whole SNR, the modeling favors a leptonic scenario in the framework of a two-zone model with an average magnetic field of 10.2 ± 0.7 μG and a limit on the maximum energy injected into protons of 2 × 1049 erg for a density of 1 cm‑3. In addition, parameter values are derived for the north?east and south?west (SW) regions of RCW 86, providing the first indication of a higher magnetic field in the SW region.
Fil: Ajello, M.. Clemson University; Estados Unidos
Fil: Baldini, L.. University Of Stanford; Estados Unidos
Fil: Barbiellini, G.. Universita Degli Studi Di Trieste; Italia
Fil: Bastieri, D.. Universita Di Padova; Italia
Fil: Bellazzini, R.. Istituto Nazionale di Fisica Nucleare; Italia
Fil: Bissaldi, E.. Istituto Nazionale di Fisica Nucleare; Italia
Fil: Bloom, E. D.. University Of Stanford; Estados Unidos
Fil: Bonino, R.. Universita degli Studi di Torino; Italia
Fil: Bottacini, E.. University Of Stanford; Estados Unidos
Fil: Brandt, T. J.. National Aeronautics And Space Administration. Goddart Institute For Space Studies; Estados Unidos
Fil: Bregeon, J.. Universite Montpellier II; Francia
Fil: Bruel, P.. Ecole Polytechnique; Francia
Fil: Buehler, R.. Deutsches Elektronen Synchrotron DESY; Alemania
Fil: Caliandro, G. A.. University Of Stanford; Estados Unidos
Fil: Cameron, R. A.. University Of Stanford; Estados Unidos
Fil: Caragiulo, M.. Universita Degli Studi Di Bari; Italia
Fil: Cavazzuti, E.. Agenzia Spaziale Italiana; Italia
Fil: Charles, E.. University Of Stanford; Estados Unidos
Fil: Chekhtman, A.. George Mason University; Estados Unidos
Fil: Ciprini, S.. Agenzia Spaziale Italiana; Italia
Fil: Cohen Tanugi, J.. Universite Montpellier II; Francia
Fil: Condon, E.. Universit´e Bordeaux; Francia
Fil: Costanza, F.. Istituto Nazionale di Fisica Nucleare; Italia
Fil: Cutini, F.. Osservatorio Astronomico di Roma; Italia
Fil: D’Ammando, F.. Universita Di Bologna; Italia
Fil: De Palma, F.. Universita Telematica Pegaso, Piazza Trieste e Trento; Italia
Fil: Desiante, R.. Universita di Udine; Italia
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: Duvidovich, Laura Patricia. 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
Fil: FERMI-LAT Collaboration.
description RCW 86 is a young supernova remnant (SNR) showing a shell-type structure at several wavelengths and is thought to be an efficient cosmic-ray (CR) accelerator. Earlier Fermi Large Area Telescope results reported the detection of γ-ray emission coincident with the position of RCW 86 but its origin (leptonic or hadronic) remained unclear due to the poor statistics. Thanks to 6.5 years of data acquired by the Fermi-LAT and the new event reconstruction Pass 8, we report the significant detection of spatially extended emission coming from RCW 86. The spectrum is described by a power-law function with a very hard photon index ({{Γ }}=1.42+/- {0.1}{{stat}}+/- {0.06}{{syst}}) in the 0.1?500 GeV range and an energy flux above 100 MeV of (2.91+/- {0.8}{{stat}}+/- {0.12}{{syst}}) × {10}-11 erg cm‑2 s‑1. Gathering all the available multiwavelength (MWL) data, we perform a broadband modeling of the nonthermal emission of RCW 86 to constrain parameters of the nearby medium and bring new hints about the origin of the γ-ray emission. For the whole SNR, the modeling favors a leptonic scenario in the framework of a two-zone model with an average magnetic field of 10.2 ± 0.7 μG and a limit on the maximum energy injected into protons of 2 × 1049 erg for a density of 1 cm‑3. In addition, parameter values are derived for the north?east and south?west (SW) regions of RCW 86, providing the first indication of a higher magnetic field in the SW region.
publishDate 2016
dc.date.none.fl_str_mv 2016-03
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/11336/18847
Ajello, M.; Baldini, L.; Barbiellini, G.; Bastieri, D.; Bellazzini, R.; et al.; Deep Morphological and Spectral Study of the SNR RCW 86 with Fermi-LAT; Iop Publishing; Astrophysical Journal; 819; 2; 3-2016; 1-13
0004-637X
CONICET Digital
CONICET
url http://hdl.handle.net/11336/18847
identifier_str_mv Ajello, M.; Baldini, L.; Barbiellini, G.; Bastieri, D.; Bellazzini, R.; et al.; Deep Morphological and Spectral Study of the SNR RCW 86 with Fermi-LAT; Iop Publishing; Astrophysical Journal; 819; 2; 3-2016; 1-13
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/https://arxiv.org/abs/1601.06534
info:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.3847/0004-637X/819/2/98/meta
info:eu-repo/semantics/altIdentifier/doi/doi:10.3847/0004-637X/819/2/98
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 Iop Publishing
publisher.none.fl_str_mv Iop Publishing
dc.source.none.fl_str_mv reponame:CONICET Digital (CONICET)
instname:Consejo Nacional de Investigaciones Científicas y Técnicas
reponame_str CONICET Digital (CONICET)
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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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