Discovery of a pulsar-powered bow shock nebula in the Small Magellanic Cloud supernova remnant DEMS5
- Autores
- Alsaberi, Rami Z. E.; Maitra, C.; Filipovic, M. D.; Bozzetto, L.M.; Haberl, F.; Maggi, P.; Sasaki, M.; Manjolovic, P.; Velovic, V.; Kavanagh, P.; Maxted, N. I.; Urosevic, D.; Rowell, G. P.; Wong, G. F.; For, B. Q.; O'Brien, A. N.; Galvin, T. J.; Staveley-Smith, L.; Norris, R. P.; Jarrett, T.; Kothes, R.; Luken, K. J.; Hurley-Walker, N.; Sano, H.; Onic, D.; Dai, S. T.; Pannuti, G.; Tothill, N. F. H.; Crawford, Evan; Yew, M.; Bojicic, I.; Dénes, H.; McClure-Griffiths, N.; Gurovich, Sebastian; Fukui, Y.
- Año de publicación
- 2019
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- We report the discovery of a new Small Magellanic Cloud pulsar wind nebula (PWN) at the edge of the supernova remnant (SNR) DEMS5. The pulsar powered object has a cometary morphology similar to the Galactic PWN analogues PSR B1951+32 and ´the mouse´. It is travelling supersonically through the interstellar medium.We estimate the pulsar kick velocity to be in the range of 700-2000 km s-1 for an age between 28 and 10 kyr. The radio spectral index for this SNR-PWN-pulsar system is flat (-0.29 ± 0.01) consistent with other similar objects. We infer that the putative pulsar has a radio spectral index of -1.8, which is typical for Galactic pulsars. We searched for dispersion measures up to 1000 cm-3 pc but found no convincing candidates with an S/N greater than 8. We produce a polarization map for this PWN at 5500 MHz and find a mean fractional polarization of P ∼ 23 per cent. The X-ray power-law spectrum (τ ∼ 2) is indicative of non-thermal synchrotron emission as is expected from PWN-pulsar system. Finally, we detect DEMS5 in infrared (IR) bands. Our IR photometric measurements strongly indicate the presence of shocked gas that is expected for SNRs. However, it is unusual to detect such IR emission in an SNR with a supersonic bow shock PWN.We also find a low-velocity HI cloud of ∼107 km s-1 that is possibly interacting with DEMS5. SNR DEMS5 is the first confirmed detection of a pulsar-powered bow shock nebula found outside the Galaxy.
Fil: Alsaberi, Rami Z. E.. Western Sydney University; Australia
Fil: Maitra, C.. Max Planck Institut Für Extraterrestrische Physik; Alemania
Fil: Filipovic, M. D.. Western Sydney University; Australia
Fil: Bozzetto, L.M.. Western Sydney University; Australia
Fil: Haberl, F.. Max Planck Institut Für Extraterrestrische Physik; Alemania
Fil: Maggi, P.. Université de Strasbourg; Francia
Fil: Sasaki, M.. Universitat Erlangen-Nuremberg; Alemania
Fil: Manjolovic, P.. Western Sydney University; Australia
Fil: Velovic, V.. University Of Belgrade; Serbia
Fil: Kavanagh, P.. Dublin Institute For Advanced Studies; Irlanda
Fil: Maxted, N. I.. University Of New South Wales (unsw) Australia; Australia
Fil: Urosevic, D.. Isaac Newton Institute Of Chile; Chile
Fil: Rowell, G. P.. University of Adelaide; Australia
Fil: Wong, G. F.. University Of New South Wales (unsw) Australia; Australia
Fil: For, B. Q.. The University Ofwestern Australia; Australia
Fil: O'Brien, A. N.. Western Sydney University; Australia
Fil: Galvin, T. J.. Western Sydney University; Australia
Fil: Staveley-Smith, L.. The University Ofwestern Australia; Australia
Fil: Norris, R. P.. Western Sydney University; Australia
Fil: Jarrett, T.. University Of Cape Town; Sudáfrica
Fil: Kothes, R.. National Research Council Canada; Canadá
Fil: Luken, K. J.. Western Sydney University; Australia
Fil: Hurley-Walker, N.. Curtin University; Australia
Fil: Sano, H.. Nagoya University; Japón
Fil: Onic, D.. University Of Belgrade; Serbia
Fil: Dai, S. T.. Australia Telescope National Facility; Australia
Fil: Pannuti, G.. Morehead State University; Estados Unidos
Fil: Tothill, N. F. H.. Western Sydney University; Australia
Fil: Crawford, Evan. Western Sydney University; Australia
Fil: Yew, M.. Western Sydney University; Australia
Fil: Bojicic, I.. Western Sydney University; Australia
Fil: Dénes, H.. Netherlands Foundation For Research In Astronomy; Bélgica
Fil: McClure-Griffiths, N.. Australian National University; Australia
Fil: Gurovich, Sebastian. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina
Fil: Fukui, Y.. Nagoya University; Japón - Materia
-
ISM: INDIVIDUAL OBJECTS: DEMS5
ISM: SUPERNOVA REMNANTS
MAGELLANIC CLOUDS
RADIATION MECHANISMS: GENERAL
RADIO CONTINUUM: ISM. - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
.jpg)
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/125653
Ver los metadatos del registro completo
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Discovery of a pulsar-powered bow shock nebula in the Small Magellanic Cloud supernova remnant DEMS5Alsaberi, Rami Z. E.Maitra, C.Filipovic, M. D.Bozzetto, L.M.Haberl, F.Maggi, P.Sasaki, M.Manjolovic, P.Velovic, V.Kavanagh, P.Maxted, N. I.Urosevic, D.Rowell, G. P.Wong, G. F.For, B. Q.O'Brien, A. N.Galvin, T. J.Staveley-Smith, L.Norris, R. P.Jarrett, T.Kothes, R.Luken, K. J.Hurley-Walker, N.Sano, H.Onic, D.Dai, S. T.Pannuti, G.Tothill, N. F. H.Crawford, EvanYew, M.Bojicic, I.Dénes, H.McClure-Griffiths, N.Gurovich, SebastianFukui, Y.ISM: INDIVIDUAL OBJECTS: DEMS5ISM: SUPERNOVA REMNANTSMAGELLANIC CLOUDSRADIATION MECHANISMS: GENERALRADIO CONTINUUM: ISM.https://purl.org/becyt/ford/1.7https://purl.org/becyt/ford/1We report the discovery of a new Small Magellanic Cloud pulsar wind nebula (PWN) at the edge of the supernova remnant (SNR) DEMS5. The pulsar powered object has a cometary morphology similar to the Galactic PWN analogues PSR B1951+32 and ´the mouse´. It is travelling supersonically through the interstellar medium.We estimate the pulsar kick velocity to be in the range of 700-2000 km s-1 for an age between 28 and 10 kyr. The radio spectral index for this SNR-PWN-pulsar system is flat (-0.29 ± 0.01) consistent with other similar objects. We infer that the putative pulsar has a radio spectral index of -1.8, which is typical for Galactic pulsars. We searched for dispersion measures up to 1000 cm-3 pc but found no convincing candidates with an S/N greater than 8. We produce a polarization map for this PWN at 5500 MHz and find a mean fractional polarization of P ∼ 23 per cent. The X-ray power-law spectrum (τ ∼ 2) is indicative of non-thermal synchrotron emission as is expected from PWN-pulsar system. Finally, we detect DEMS5 in infrared (IR) bands. Our IR photometric measurements strongly indicate the presence of shocked gas that is expected for SNRs. However, it is unusual to detect such IR emission in an SNR with a supersonic bow shock PWN.We also find a low-velocity HI cloud of ∼107 km s-1 that is possibly interacting with DEMS5. SNR DEMS5 is the first confirmed detection of a pulsar-powered bow shock nebula found outside the Galaxy.Fil: Alsaberi, Rami Z. E.. Western Sydney University; AustraliaFil: Maitra, C.. Max Planck Institut Für Extraterrestrische Physik; AlemaniaFil: Filipovic, M. D.. Western Sydney University; AustraliaFil: Bozzetto, L.M.. Western Sydney University; AustraliaFil: Haberl, F.. Max Planck Institut Für Extraterrestrische Physik; AlemaniaFil: Maggi, P.. Université de Strasbourg; FranciaFil: Sasaki, M.. Universitat Erlangen-Nuremberg; AlemaniaFil: Manjolovic, P.. Western Sydney University; AustraliaFil: Velovic, V.. University Of Belgrade; SerbiaFil: Kavanagh, P.. Dublin Institute For Advanced Studies; IrlandaFil: Maxted, N. I.. University Of New South Wales (unsw) Australia; AustraliaFil: Urosevic, D.. Isaac Newton Institute Of Chile; ChileFil: Rowell, G. P.. University of Adelaide; AustraliaFil: Wong, G. F.. University Of New South Wales (unsw) Australia; AustraliaFil: For, B. Q.. The University Ofwestern Australia; AustraliaFil: O'Brien, A. N.. Western Sydney University; AustraliaFil: Galvin, T. J.. Western Sydney University; AustraliaFil: Staveley-Smith, L.. The University Ofwestern Australia; AustraliaFil: Norris, R. P.. Western Sydney University; AustraliaFil: Jarrett, T.. University Of Cape Town; SudáfricaFil: Kothes, R.. National Research Council Canada; CanadáFil: Luken, K. J.. Western Sydney University; AustraliaFil: Hurley-Walker, N.. Curtin University; AustraliaFil: Sano, H.. Nagoya University; JapónFil: Onic, D.. University Of Belgrade; SerbiaFil: Dai, S. T.. Australia Telescope National Facility; AustraliaFil: Pannuti, G.. Morehead State University; Estados UnidosFil: Tothill, N. F. H.. Western Sydney University; AustraliaFil: Crawford, Evan. Western Sydney University; AustraliaFil: Yew, M.. Western Sydney University; AustraliaFil: Bojicic, I.. Western Sydney University; AustraliaFil: Dénes, H.. Netherlands Foundation For Research In Astronomy; BélgicaFil: McClure-Griffiths, N.. Australian National University; AustraliaFil: Gurovich, Sebastian. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; ArgentinaFil: Fukui, Y.. Nagoya University; JapónWiley Blackwell Publishing, Inc2019-06info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/125653Alsaberi, Rami Z. E.; Maitra, C.; Filipovic, M. D.; Bozzetto, L.M.; Haberl, F.; et al.; Discovery of a pulsar-powered bow shock nebula in the Small Magellanic Cloud supernova remnant DEMS5; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 486; 2; 6-2019; 2507-25240035-8711CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stz971info:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article-abstract/486/2/2507/5432366info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-22T11:04:53Zoai:ri.conicet.gov.ar:11336/125653instacron: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:34982025-10-22 11:04:53.537CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
| dc.title.none.fl_str_mv |
Discovery of a pulsar-powered bow shock nebula in the Small Magellanic Cloud supernova remnant DEMS5 |
| title |
Discovery of a pulsar-powered bow shock nebula in the Small Magellanic Cloud supernova remnant DEMS5 |
| spellingShingle |
Discovery of a pulsar-powered bow shock nebula in the Small Magellanic Cloud supernova remnant DEMS5 Alsaberi, Rami Z. E. ISM: INDIVIDUAL OBJECTS: DEMS5 ISM: SUPERNOVA REMNANTS MAGELLANIC CLOUDS RADIATION MECHANISMS: GENERAL RADIO CONTINUUM: ISM. |
| title_short |
Discovery of a pulsar-powered bow shock nebula in the Small Magellanic Cloud supernova remnant DEMS5 |
| title_full |
Discovery of a pulsar-powered bow shock nebula in the Small Magellanic Cloud supernova remnant DEMS5 |
| title_fullStr |
Discovery of a pulsar-powered bow shock nebula in the Small Magellanic Cloud supernova remnant DEMS5 |
| title_full_unstemmed |
Discovery of a pulsar-powered bow shock nebula in the Small Magellanic Cloud supernova remnant DEMS5 |
| title_sort |
Discovery of a pulsar-powered bow shock nebula in the Small Magellanic Cloud supernova remnant DEMS5 |
| dc.creator.none.fl_str_mv |
Alsaberi, Rami Z. E. Maitra, C. Filipovic, M. D. Bozzetto, L.M. Haberl, F. Maggi, P. Sasaki, M. Manjolovic, P. Velovic, V. Kavanagh, P. Maxted, N. I. Urosevic, D. Rowell, G. P. Wong, G. F. For, B. Q. O'Brien, A. N. Galvin, T. J. Staveley-Smith, L. Norris, R. P. Jarrett, T. Kothes, R. Luken, K. J. Hurley-Walker, N. Sano, H. Onic, D. Dai, S. T. Pannuti, G. Tothill, N. F. H. Crawford, Evan Yew, M. Bojicic, I. Dénes, H. McClure-Griffiths, N. Gurovich, Sebastian Fukui, Y. |
| author |
Alsaberi, Rami Z. E. |
| author_facet |
Alsaberi, Rami Z. E. Maitra, C. Filipovic, M. D. Bozzetto, L.M. Haberl, F. Maggi, P. Sasaki, M. Manjolovic, P. Velovic, V. Kavanagh, P. Maxted, N. I. Urosevic, D. Rowell, G. P. Wong, G. F. For, B. Q. O'Brien, A. N. Galvin, T. J. Staveley-Smith, L. Norris, R. P. Jarrett, T. Kothes, R. Luken, K. J. Hurley-Walker, N. Sano, H. Onic, D. Dai, S. T. Pannuti, G. Tothill, N. F. H. Crawford, Evan Yew, M. Bojicic, I. Dénes, H. McClure-Griffiths, N. Gurovich, Sebastian Fukui, Y. |
| author_role |
author |
| author2 |
Maitra, C. Filipovic, M. D. Bozzetto, L.M. Haberl, F. Maggi, P. Sasaki, M. Manjolovic, P. Velovic, V. Kavanagh, P. Maxted, N. I. Urosevic, D. Rowell, G. P. Wong, G. F. For, B. Q. O'Brien, A. N. Galvin, T. J. Staveley-Smith, L. Norris, R. P. Jarrett, T. Kothes, R. Luken, K. J. Hurley-Walker, N. Sano, H. Onic, D. Dai, S. T. Pannuti, G. Tothill, N. F. H. Crawford, Evan Yew, M. Bojicic, I. Dénes, H. McClure-Griffiths, N. Gurovich, Sebastian Fukui, Y. |
| 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 author author author author |
| dc.subject.none.fl_str_mv |
ISM: INDIVIDUAL OBJECTS: DEMS5 ISM: SUPERNOVA REMNANTS MAGELLANIC CLOUDS RADIATION MECHANISMS: GENERAL RADIO CONTINUUM: ISM. |
| topic |
ISM: INDIVIDUAL OBJECTS: DEMS5 ISM: SUPERNOVA REMNANTS MAGELLANIC CLOUDS RADIATION MECHANISMS: GENERAL RADIO CONTINUUM: ISM. |
| purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.7 https://purl.org/becyt/ford/1 |
| dc.description.none.fl_txt_mv |
We report the discovery of a new Small Magellanic Cloud pulsar wind nebula (PWN) at the edge of the supernova remnant (SNR) DEMS5. The pulsar powered object has a cometary morphology similar to the Galactic PWN analogues PSR B1951+32 and ´the mouse´. It is travelling supersonically through the interstellar medium.We estimate the pulsar kick velocity to be in the range of 700-2000 km s-1 for an age between 28 and 10 kyr. The radio spectral index for this SNR-PWN-pulsar system is flat (-0.29 ± 0.01) consistent with other similar objects. We infer that the putative pulsar has a radio spectral index of -1.8, which is typical for Galactic pulsars. We searched for dispersion measures up to 1000 cm-3 pc but found no convincing candidates with an S/N greater than 8. We produce a polarization map for this PWN at 5500 MHz and find a mean fractional polarization of P ∼ 23 per cent. The X-ray power-law spectrum (τ ∼ 2) is indicative of non-thermal synchrotron emission as is expected from PWN-pulsar system. Finally, we detect DEMS5 in infrared (IR) bands. Our IR photometric measurements strongly indicate the presence of shocked gas that is expected for SNRs. However, it is unusual to detect such IR emission in an SNR with a supersonic bow shock PWN.We also find a low-velocity HI cloud of ∼107 km s-1 that is possibly interacting with DEMS5. SNR DEMS5 is the first confirmed detection of a pulsar-powered bow shock nebula found outside the Galaxy. Fil: Alsaberi, Rami Z. E.. Western Sydney University; Australia Fil: Maitra, C.. Max Planck Institut Für Extraterrestrische Physik; Alemania Fil: Filipovic, M. D.. Western Sydney University; Australia Fil: Bozzetto, L.M.. Western Sydney University; Australia Fil: Haberl, F.. Max Planck Institut Für Extraterrestrische Physik; Alemania Fil: Maggi, P.. Université de Strasbourg; Francia Fil: Sasaki, M.. Universitat Erlangen-Nuremberg; Alemania Fil: Manjolovic, P.. Western Sydney University; Australia Fil: Velovic, V.. University Of Belgrade; Serbia Fil: Kavanagh, P.. Dublin Institute For Advanced Studies; Irlanda Fil: Maxted, N. I.. University Of New South Wales (unsw) Australia; Australia Fil: Urosevic, D.. Isaac Newton Institute Of Chile; Chile Fil: Rowell, G. P.. University of Adelaide; Australia Fil: Wong, G. F.. University Of New South Wales (unsw) Australia; Australia Fil: For, B. Q.. The University Ofwestern Australia; Australia Fil: O'Brien, A. N.. Western Sydney University; Australia Fil: Galvin, T. J.. Western Sydney University; Australia Fil: Staveley-Smith, L.. The University Ofwestern Australia; Australia Fil: Norris, R. P.. Western Sydney University; Australia Fil: Jarrett, T.. University Of Cape Town; Sudáfrica Fil: Kothes, R.. National Research Council Canada; Canadá Fil: Luken, K. J.. Western Sydney University; Australia Fil: Hurley-Walker, N.. Curtin University; Australia Fil: Sano, H.. Nagoya University; Japón Fil: Onic, D.. University Of Belgrade; Serbia Fil: Dai, S. T.. Australia Telescope National Facility; Australia Fil: Pannuti, G.. Morehead State University; Estados Unidos Fil: Tothill, N. F. H.. Western Sydney University; Australia Fil: Crawford, Evan. Western Sydney University; Australia Fil: Yew, M.. Western Sydney University; Australia Fil: Bojicic, I.. Western Sydney University; Australia Fil: Dénes, H.. Netherlands Foundation For Research In Astronomy; Bélgica Fil: McClure-Griffiths, N.. Australian National University; Australia Fil: Gurovich, Sebastian. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina Fil: Fukui, Y.. Nagoya University; Japón |
| description |
We report the discovery of a new Small Magellanic Cloud pulsar wind nebula (PWN) at the edge of the supernova remnant (SNR) DEMS5. The pulsar powered object has a cometary morphology similar to the Galactic PWN analogues PSR B1951+32 and ´the mouse´. It is travelling supersonically through the interstellar medium.We estimate the pulsar kick velocity to be in the range of 700-2000 km s-1 for an age between 28 and 10 kyr. The radio spectral index for this SNR-PWN-pulsar system is flat (-0.29 ± 0.01) consistent with other similar objects. We infer that the putative pulsar has a radio spectral index of -1.8, which is typical for Galactic pulsars. We searched for dispersion measures up to 1000 cm-3 pc but found no convincing candidates with an S/N greater than 8. We produce a polarization map for this PWN at 5500 MHz and find a mean fractional polarization of P ∼ 23 per cent. The X-ray power-law spectrum (τ ∼ 2) is indicative of non-thermal synchrotron emission as is expected from PWN-pulsar system. Finally, we detect DEMS5 in infrared (IR) bands. Our IR photometric measurements strongly indicate the presence of shocked gas that is expected for SNRs. However, it is unusual to detect such IR emission in an SNR with a supersonic bow shock PWN.We also find a low-velocity HI cloud of ∼107 km s-1 that is possibly interacting with DEMS5. SNR DEMS5 is the first confirmed detection of a pulsar-powered bow shock nebula found outside the Galaxy. |
| publishDate |
2019 |
| dc.date.none.fl_str_mv |
2019-06 |
| 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/11336/125653 Alsaberi, Rami Z. E.; Maitra, C.; Filipovic, M. D.; Bozzetto, L.M.; Haberl, F.; et al.; Discovery of a pulsar-powered bow shock nebula in the Small Magellanic Cloud supernova remnant DEMS5; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 486; 2; 6-2019; 2507-2524 0035-8711 CONICET Digital CONICET |
| url |
http://hdl.handle.net/11336/125653 |
| identifier_str_mv |
Alsaberi, Rami Z. E.; Maitra, C.; Filipovic, M. D.; Bozzetto, L.M.; Haberl, F.; et al.; Discovery of a pulsar-powered bow shock nebula in the Small Magellanic Cloud supernova remnant DEMS5; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 486; 2; 6-2019; 2507-2524 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/doi/10.1093/mnras/stz971 info:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article-abstract/486/2/2507/5432366 |
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info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
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openAccess |
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https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
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application/pdf application/pdf |
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Wiley Blackwell Publishing, Inc |
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Wiley Blackwell Publishing, Inc |
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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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