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
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/18847
Ver los metadatos del registro completo
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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) |
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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13.070432 |