Thermal emission, shock modification, and X-ray emitting ejecta in SN 1006
- Autores
- Miceli, M.; Bocchino, F.; Iakubovskyi, D.; Orlando, S.; Telezhinsky, I.; Kirsch, M. G. F; Petruk, O.; Dubner, Gloria Mabel; Castelletti, Gabriela Marta
- Año de publicación
- 2009
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- Context: Efficient particle acceleration can modify the structure of supernova remnants. We present the results of a combined analysis of the XMM-Newton EPIC archive observations of SN 1006. Aims: We attempt to describe the spatial distribution of the physical and chemical properties of the X-ray emitting plasma at the shock front. We investigate the contribution of thermal and non-thermal emission to the X-ray spectrum at the rim of the remnant to study how the acceleration processes affect the X-ray emitting plasma. Methods: We perform a spatially resolved spectral analysis of a set of regions covering the entire rim of the shell and we apply our results in producing a count-rate image of the ?pure? thermal emission of SN 1006 in the 0.5-0.8 keV energy band (subtracting the non-thermal contribution). This image differs significantly from the total image in the same band, especially close to the bright limbs. Results: We find that thermal X-ray emission can be associated with the ejecta and study the azimuthal variation in the physical and chemical properties of the ejecta by identifying anisotropies in the temperature and chemical composition. By employing our thermal image, we trace the position of the contact discontinuity over the entire shell and compare it with that expected from 3D MHD models of SNRs with an unmodified shock. Conclusions: We conclude that the shock is modified everywhere in the rim and that the aspect angle between the interstellar magnetic field and the line of sight is significantly lower than 90°.
Fil: Miceli, M.. Università di Palermo; Italia
Fil: Bocchino, F.. Istituto Nazionale Di Astrofísica. Osservatorio Astronómico Di Palermo; Italia
Fil: Iakubovskyi, D.. Bogolyubov Institute for Theoretical Physics; Ucrania
Fil: Orlando, S.. Istituto Nazionale Di Astrofísica. Osservatorio Astronómico Di Palermo; Italia
Fil: Telezhinsky, I.. Astronomical Observatory; Ucrania
Fil: Kirsch, M. G. F. European Space Operations Centre; Alemania
Fil: Petruk, O.. National University; Ucrania
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: Castelletti, Gabriela Marta. 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 - Materia
-
X-RAYS: ISM
ISM: SUPERNOVA REMNANTS
ISM:INDIVIDUAL OBJECTS: SN 1006 - 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:11336/21926
Ver los metadatos del registro completo
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Thermal emission, shock modification, and X-ray emitting ejecta in SN 1006Miceli, M.Bocchino, F.Iakubovskyi, D.Orlando, S.Telezhinsky, I.Kirsch, M. G. FPetruk, O.Dubner, Gloria MabelCastelletti, Gabriela MartaX-RAYS: ISMISM: SUPERNOVA REMNANTSISM:INDIVIDUAL OBJECTS: SN 1006https://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Context: Efficient particle acceleration can modify the structure of supernova remnants. We present the results of a combined analysis of the XMM-Newton EPIC archive observations of SN 1006. Aims: We attempt to describe the spatial distribution of the physical and chemical properties of the X-ray emitting plasma at the shock front. We investigate the contribution of thermal and non-thermal emission to the X-ray spectrum at the rim of the remnant to study how the acceleration processes affect the X-ray emitting plasma. Methods: We perform a spatially resolved spectral analysis of a set of regions covering the entire rim of the shell and we apply our results in producing a count-rate image of the ?pure? thermal emission of SN 1006 in the 0.5-0.8 keV energy band (subtracting the non-thermal contribution). This image differs significantly from the total image in the same band, especially close to the bright limbs. Results: We find that thermal X-ray emission can be associated with the ejecta and study the azimuthal variation in the physical and chemical properties of the ejecta by identifying anisotropies in the temperature and chemical composition. By employing our thermal image, we trace the position of the contact discontinuity over the entire shell and compare it with that expected from 3D MHD models of SNRs with an unmodified shock. Conclusions: We conclude that the shock is modified everywhere in the rim and that the aspect angle between the interstellar magnetic field and the line of sight is significantly lower than 90°.Fil: Miceli, M.. Università di Palermo; ItaliaFil: Bocchino, F.. Istituto Nazionale Di Astrofísica. Osservatorio Astronómico Di Palermo; ItaliaFil: Iakubovskyi, D.. Bogolyubov Institute for Theoretical Physics; UcraniaFil: Orlando, S.. Istituto Nazionale Di Astrofísica. Osservatorio Astronómico Di Palermo; ItaliaFil: Telezhinsky, I.. Astronomical Observatory; UcraniaFil: Kirsch, M. G. F. European Space Operations Centre; AlemaniaFil: Petruk, O.. National University; UcraniaFil: 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: Castelletti, Gabriela Marta. 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; ArgentinaEDP Sciences2009-12info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/21926Miceli, M.; Bocchino, F.; Iakubovskyi, D.; Orlando, S.; Telezhinsky, I.; et al.; Thermal emission, shock modification, and X-ray emitting ejecta in SN 1006; EDP Sciences; Astronomy and Astrophysics; 501; 1; 12-2009; 239-2490004-6361CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361/200811505info:eu-repo/semantics/altIdentifier/url/https://www.aanda.org/articles/aa/abs/2009/25/aa11505-08/aa11505-08.htmlinfo:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/0903.3392info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:47:54Zoai:ri.conicet.gov.ar:11336/21926instacron: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 10:47:54.599CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
| dc.title.none.fl_str_mv |
Thermal emission, shock modification, and X-ray emitting ejecta in SN 1006 |
| title |
Thermal emission, shock modification, and X-ray emitting ejecta in SN 1006 |
| spellingShingle |
Thermal emission, shock modification, and X-ray emitting ejecta in SN 1006 Miceli, M. X-RAYS: ISM ISM: SUPERNOVA REMNANTS ISM:INDIVIDUAL OBJECTS: SN 1006 |
| title_short |
Thermal emission, shock modification, and X-ray emitting ejecta in SN 1006 |
| title_full |
Thermal emission, shock modification, and X-ray emitting ejecta in SN 1006 |
| title_fullStr |
Thermal emission, shock modification, and X-ray emitting ejecta in SN 1006 |
| title_full_unstemmed |
Thermal emission, shock modification, and X-ray emitting ejecta in SN 1006 |
| title_sort |
Thermal emission, shock modification, and X-ray emitting ejecta in SN 1006 |
| dc.creator.none.fl_str_mv |
Miceli, M. Bocchino, F. Iakubovskyi, D. Orlando, S. Telezhinsky, I. Kirsch, M. G. F Petruk, O. Dubner, Gloria Mabel Castelletti, Gabriela Marta |
| author |
Miceli, M. |
| author_facet |
Miceli, M. Bocchino, F. Iakubovskyi, D. Orlando, S. Telezhinsky, I. Kirsch, M. G. F Petruk, O. Dubner, Gloria Mabel Castelletti, Gabriela Marta |
| author_role |
author |
| author2 |
Bocchino, F. Iakubovskyi, D. Orlando, S. Telezhinsky, I. Kirsch, M. G. F Petruk, O. Dubner, Gloria Mabel Castelletti, Gabriela Marta |
| author2_role |
author author author author author author author author |
| dc.subject.none.fl_str_mv |
X-RAYS: ISM ISM: SUPERNOVA REMNANTS ISM:INDIVIDUAL OBJECTS: SN 1006 |
| topic |
X-RAYS: ISM ISM: SUPERNOVA REMNANTS ISM:INDIVIDUAL OBJECTS: SN 1006 |
| purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
| dc.description.none.fl_txt_mv |
Context: Efficient particle acceleration can modify the structure of supernova remnants. We present the results of a combined analysis of the XMM-Newton EPIC archive observations of SN 1006. Aims: We attempt to describe the spatial distribution of the physical and chemical properties of the X-ray emitting plasma at the shock front. We investigate the contribution of thermal and non-thermal emission to the X-ray spectrum at the rim of the remnant to study how the acceleration processes affect the X-ray emitting plasma. Methods: We perform a spatially resolved spectral analysis of a set of regions covering the entire rim of the shell and we apply our results in producing a count-rate image of the ?pure? thermal emission of SN 1006 in the 0.5-0.8 keV energy band (subtracting the non-thermal contribution). This image differs significantly from the total image in the same band, especially close to the bright limbs. Results: We find that thermal X-ray emission can be associated with the ejecta and study the azimuthal variation in the physical and chemical properties of the ejecta by identifying anisotropies in the temperature and chemical composition. By employing our thermal image, we trace the position of the contact discontinuity over the entire shell and compare it with that expected from 3D MHD models of SNRs with an unmodified shock. Conclusions: We conclude that the shock is modified everywhere in the rim and that the aspect angle between the interstellar magnetic field and the line of sight is significantly lower than 90°. Fil: Miceli, M.. Università di Palermo; Italia Fil: Bocchino, F.. Istituto Nazionale Di Astrofísica. Osservatorio Astronómico Di Palermo; Italia Fil: Iakubovskyi, D.. Bogolyubov Institute for Theoretical Physics; Ucrania Fil: Orlando, S.. Istituto Nazionale Di Astrofísica. Osservatorio Astronómico Di Palermo; Italia Fil: Telezhinsky, I.. Astronomical Observatory; Ucrania Fil: Kirsch, M. G. F. European Space Operations Centre; Alemania Fil: Petruk, O.. National University; Ucrania 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: Castelletti, Gabriela Marta. 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 |
| description |
Context: Efficient particle acceleration can modify the structure of supernova remnants. We present the results of a combined analysis of the XMM-Newton EPIC archive observations of SN 1006. Aims: We attempt to describe the spatial distribution of the physical and chemical properties of the X-ray emitting plasma at the shock front. We investigate the contribution of thermal and non-thermal emission to the X-ray spectrum at the rim of the remnant to study how the acceleration processes affect the X-ray emitting plasma. Methods: We perform a spatially resolved spectral analysis of a set of regions covering the entire rim of the shell and we apply our results in producing a count-rate image of the ?pure? thermal emission of SN 1006 in the 0.5-0.8 keV energy band (subtracting the non-thermal contribution). This image differs significantly from the total image in the same band, especially close to the bright limbs. Results: We find that thermal X-ray emission can be associated with the ejecta and study the azimuthal variation in the physical and chemical properties of the ejecta by identifying anisotropies in the temperature and chemical composition. By employing our thermal image, we trace the position of the contact discontinuity over the entire shell and compare it with that expected from 3D MHD models of SNRs with an unmodified shock. Conclusions: We conclude that the shock is modified everywhere in the rim and that the aspect angle between the interstellar magnetic field and the line of sight is significantly lower than 90°. |
| publishDate |
2009 |
| dc.date.none.fl_str_mv |
2009-12 |
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info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
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article |
| status_str |
publishedVersion |
| dc.identifier.none.fl_str_mv |
http://hdl.handle.net/11336/21926 Miceli, M.; Bocchino, F.; Iakubovskyi, D.; Orlando, S.; Telezhinsky, I.; et al.; Thermal emission, shock modification, and X-ray emitting ejecta in SN 1006; EDP Sciences; Astronomy and Astrophysics; 501; 1; 12-2009; 239-249 0004-6361 CONICET Digital CONICET |
| url |
http://hdl.handle.net/11336/21926 |
| identifier_str_mv |
Miceli, M.; Bocchino, F.; Iakubovskyi, D.; Orlando, S.; Telezhinsky, I.; et al.; Thermal emission, shock modification, and X-ray emitting ejecta in SN 1006; EDP Sciences; Astronomy and Astrophysics; 501; 1; 12-2009; 239-249 0004-6361 CONICET Digital CONICET |
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eng |
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eng |
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info:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361/200811505 info:eu-repo/semantics/altIdentifier/url/https://www.aanda.org/articles/aa/abs/2009/25/aa11505-08/aa11505-08.html info:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/0903.3392 |
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EDP Sciences |
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