XMM-Newton detection of the supernova remnant G304.6+0.1 (Kes 17)
- Autores
- Combi, Jorge A.; Albacete Colombo, Juan Facundo; Sánchez Ayaso, Estrella; Romero, Gustavo E.; Marti, J.; Luque Escamilla, P. L.; Muñoz Arjonilla, A. J.; Sánchez Sutil, J. R.; López Santiago, J.
- Año de publicación
- 2010
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- Fil: Combi, Jorge A. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico la Plata. Instituto Argentino de Radioastronomia (i); Argentina.
Fil: Combi, Jorge A. Universidad de Jaén; España
Fil: Combi, Jorge A. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina
Fil: Albacete Colombo, Juan F. Universidad Nacional del Comahue; Argentina
Fil: Sánchez Ayaso, Estrella. Universidad de Jaén; España
Fil: Romero, Gustavo E. 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: Romero, Gustavo E. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina
Fil: Marti, J. Universidad de Jaén; España
Fil: Luque Escamilla, P. L. Escuela Politécnica Superior, Universidad de Jaén. Departamento de Ingeniería Mecánica y Minera; España
Fil: Muñoz Arjonilla, A. J. Escuela Politécnica Superior, Universidad de Jaén. Departamento de Ingeniería Mecánica y Minera; España
Fil: Sánchez Sutil, J. R. Escuela Politécnica Superior, Universidad de Jaén. Departamento de Ingeniería Mecánica y Minera; España
Fil: López Santiago, J. Universidad Complutense de Madrid. Departamento de Astrofísica y Ciencias de la Atmósfera; España
Aims. We report the first detailed X-ray study of the supernova remnant (SNR) G304.6+0.1, achieved with the XMM-Newton mission. Methods. The powerful imaging capability of XMM-Newton was used to study the X-ray characteristics of the remnant at different energy ranges. The X-ray morphology and spectral properties were analyzed. In addittion, radio and mid-infrared data obtained with the Molonglo Observatory Synthesis Telescope and the Spitzer Space Telescope were used to study the association with the detected X-ray emission and to understand the structure of the SNR at differents wavelengths. Results. The SNR shows an extended and arc-like internal structure in the X-ray band without a compact point-like source inside the remnant. We find a high column density of NH in the range 2.5–3.5 × 1022 cm−2, which supports a relatively distant location (d ≥ 9.7 kpc). The X-ray spectrum exhibits at least three emission lines, indicating that the X-ray emission has a thin thermal plasma origin, although a non-thermal contribution cannot be discarded. The spectra of three different regions (north, center and south) are well represented by a combination of a non-equilibrium ionization (PSHOCK) and a power-law (PL) model. The mid-infrared observations show a bright filamentary structure along the north-south direction coincident with the NW radio shell. This suggests that Kes 17 is propagating in a non-uniform environment with high density and that the shock front is interacting with several adjacent massive molecular clouds. The good correspondence of radio and mid-infrared emissions suggests that the filamentary features are caused by shock compression. The X-ray characteristics and well-known radio parameters indicate that G304.6+0.1 is a middle-aged SNR (2.8−6.4) × 104 yr old and a new member of the recently proposed group of mixed-morphology SNRs. - Materia
-
Ciencias Exactas y Naturales
ISM: Individual Objects: G304.6+0.1
ISM: Supernova Remnants
X-rays: ISM
Radiation Mechanisms: Thermal
Ciencias Exactas y Naturales - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/4.0/
- Repositorio
- Institución
- Universidad Nacional de Río Negro
- OAI Identificador
- oai:rid.unrn.edu.ar:20.500.12049/2507
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XMM-Newton detection of the supernova remnant G304.6+0.1 (Kes 17)Combi, Jorge A.Albacete Colombo, Juan FacundoSánchez Ayaso, EstrellaRomero, Gustavo E.Marti, J.Luque Escamilla, P. L.Muñoz Arjonilla, A. J.Sánchez Sutil, J. R.López Santiago, J.Ciencias Exactas y NaturalesISM: Individual Objects: G304.6+0.1ISM: Supernova RemnantsX-rays: ISMRadiation Mechanisms: ThermalCiencias Exactas y NaturalesFil: Combi, Jorge A. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico la Plata. Instituto Argentino de Radioastronomia (i); Argentina.Fil: Combi, Jorge A. Universidad de Jaén; EspañaFil: Combi, Jorge A. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; ArgentinaFil: Albacete Colombo, Juan F. Universidad Nacional del Comahue; ArgentinaFil: Sánchez Ayaso, Estrella. Universidad de Jaén; EspañaFil: Romero, Gustavo E. 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: Romero, Gustavo E. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; ArgentinaFil: Marti, J. Universidad de Jaén; EspañaFil: Luque Escamilla, P. L. Escuela Politécnica Superior, Universidad de Jaén. Departamento de Ingeniería Mecánica y Minera; EspañaFil: Muñoz Arjonilla, A. J. Escuela Politécnica Superior, Universidad de Jaén. Departamento de Ingeniería Mecánica y Minera; EspañaFil: Sánchez Sutil, J. R. Escuela Politécnica Superior, Universidad de Jaén. Departamento de Ingeniería Mecánica y Minera; EspañaFil: López Santiago, J. Universidad Complutense de Madrid. Departamento de Astrofísica y Ciencias de la Atmósfera; EspañaAims. We report the first detailed X-ray study of the supernova remnant (SNR) G304.6+0.1, achieved with the XMM-Newton mission. Methods. The powerful imaging capability of XMM-Newton was used to study the X-ray characteristics of the remnant at different energy ranges. The X-ray morphology and spectral properties were analyzed. In addittion, radio and mid-infrared data obtained with the Molonglo Observatory Synthesis Telescope and the Spitzer Space Telescope were used to study the association with the detected X-ray emission and to understand the structure of the SNR at differents wavelengths. Results. The SNR shows an extended and arc-like internal structure in the X-ray band without a compact point-like source inside the remnant. We find a high column density of NH in the range 2.5–3.5 × 1022 cm−2, which supports a relatively distant location (d ≥ 9.7 kpc). The X-ray spectrum exhibits at least three emission lines, indicating that the X-ray emission has a thin thermal plasma origin, although a non-thermal contribution cannot be discarded. The spectra of three different regions (north, center and south) are well represented by a combination of a non-equilibrium ionization (PSHOCK) and a power-law (PL) model. The mid-infrared observations show a bright filamentary structure along the north-south direction coincident with the NW radio shell. This suggests that Kes 17 is propagating in a non-uniform environment with high density and that the shock front is interacting with several adjacent massive molecular clouds. The good correspondence of radio and mid-infrared emissions suggests that the filamentary features are caused by shock compression. The X-ray characteristics and well-known radio parameters indicate that G304.6+0.1 is a middle-aged SNR (2.8−6.4) × 104 yr old and a new member of the recently proposed group of mixed-morphology SNRs.Edp Sciences2010-09-13info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfCombi, Jorge A., Albacete Colombo, Juan F., Sánchez Ayaso, Estrella, Romero, Gustavo E., Marti, J. (2010). XMM-Newton detection of the supernova remnant G304.6+0.1 (Kes 17); Edp Sciences; Astronomy And Astrophysics1432-07460004-6361https://www.aanda.org/articles/aa/abs/2010/15/aa13935-09/aa13935-09.htmlhttps://rid.unrn.edu.ar/jspui/handle/20.500.12049/2507http://dx.doi.org/10.1051/0004-6361/200913935http://hdl.handle.net/11336/18905eng523Astronomy And Astrophysicsinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/4.0/reponame:RID-UNRN (UNRN)instname:Universidad Nacional de Río Negro2025-10-23T11:17:41Zoai:rid.unrn.edu.ar:20.500.12049/2507instacron:UNRNInstitucionalhttps://rid.unrn.edu.ar/jspui/Universidad públicaNo correspondehttps://rid.unrn.edu.ar/oai/snrdrid@unrn.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:43692025-10-23 11:17:41.816RID-UNRN (UNRN) - Universidad Nacional de Río Negrofalse |
dc.title.none.fl_str_mv |
XMM-Newton detection of the supernova remnant G304.6+0.1 (Kes 17) |
title |
XMM-Newton detection of the supernova remnant G304.6+0.1 (Kes 17) |
spellingShingle |
XMM-Newton detection of the supernova remnant G304.6+0.1 (Kes 17) Combi, Jorge A. Ciencias Exactas y Naturales ISM: Individual Objects: G304.6+0.1 ISM: Supernova Remnants X-rays: ISM Radiation Mechanisms: Thermal Ciencias Exactas y Naturales |
title_short |
XMM-Newton detection of the supernova remnant G304.6+0.1 (Kes 17) |
title_full |
XMM-Newton detection of the supernova remnant G304.6+0.1 (Kes 17) |
title_fullStr |
XMM-Newton detection of the supernova remnant G304.6+0.1 (Kes 17) |
title_full_unstemmed |
XMM-Newton detection of the supernova remnant G304.6+0.1 (Kes 17) |
title_sort |
XMM-Newton detection of the supernova remnant G304.6+0.1 (Kes 17) |
dc.creator.none.fl_str_mv |
Combi, Jorge A. Albacete Colombo, Juan Facundo Sánchez Ayaso, Estrella Romero, Gustavo E. Marti, J. Luque Escamilla, P. L. Muñoz Arjonilla, A. J. Sánchez Sutil, J. R. López Santiago, J. |
author |
Combi, Jorge A. |
author_facet |
Combi, Jorge A. Albacete Colombo, Juan Facundo Sánchez Ayaso, Estrella Romero, Gustavo E. Marti, J. Luque Escamilla, P. L. Muñoz Arjonilla, A. J. Sánchez Sutil, J. R. López Santiago, J. |
author_role |
author |
author2 |
Albacete Colombo, Juan Facundo Sánchez Ayaso, Estrella Romero, Gustavo E. Marti, J. Luque Escamilla, P. L. Muñoz Arjonilla, A. J. Sánchez Sutil, J. R. López Santiago, J. |
author2_role |
author author author author author author author author |
dc.subject.none.fl_str_mv |
Ciencias Exactas y Naturales ISM: Individual Objects: G304.6+0.1 ISM: Supernova Remnants X-rays: ISM Radiation Mechanisms: Thermal Ciencias Exactas y Naturales |
topic |
Ciencias Exactas y Naturales ISM: Individual Objects: G304.6+0.1 ISM: Supernova Remnants X-rays: ISM Radiation Mechanisms: Thermal Ciencias Exactas y Naturales |
dc.description.none.fl_txt_mv |
Fil: Combi, Jorge A. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico la Plata. Instituto Argentino de Radioastronomia (i); Argentina. Fil: Combi, Jorge A. Universidad de Jaén; España Fil: Combi, Jorge A. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina Fil: Albacete Colombo, Juan F. Universidad Nacional del Comahue; Argentina Fil: Sánchez Ayaso, Estrella. Universidad de Jaén; España Fil: Romero, Gustavo E. 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: Romero, Gustavo E. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina Fil: Marti, J. Universidad de Jaén; España Fil: Luque Escamilla, P. L. Escuela Politécnica Superior, Universidad de Jaén. Departamento de Ingeniería Mecánica y Minera; España Fil: Muñoz Arjonilla, A. J. Escuela Politécnica Superior, Universidad de Jaén. Departamento de Ingeniería Mecánica y Minera; España Fil: Sánchez Sutil, J. R. Escuela Politécnica Superior, Universidad de Jaén. Departamento de Ingeniería Mecánica y Minera; España Fil: López Santiago, J. Universidad Complutense de Madrid. Departamento de Astrofísica y Ciencias de la Atmósfera; España Aims. We report the first detailed X-ray study of the supernova remnant (SNR) G304.6+0.1, achieved with the XMM-Newton mission. Methods. The powerful imaging capability of XMM-Newton was used to study the X-ray characteristics of the remnant at different energy ranges. The X-ray morphology and spectral properties were analyzed. In addittion, radio and mid-infrared data obtained with the Molonglo Observatory Synthesis Telescope and the Spitzer Space Telescope were used to study the association with the detected X-ray emission and to understand the structure of the SNR at differents wavelengths. Results. The SNR shows an extended and arc-like internal structure in the X-ray band without a compact point-like source inside the remnant. We find a high column density of NH in the range 2.5–3.5 × 1022 cm−2, which supports a relatively distant location (d ≥ 9.7 kpc). The X-ray spectrum exhibits at least three emission lines, indicating that the X-ray emission has a thin thermal plasma origin, although a non-thermal contribution cannot be discarded. The spectra of three different regions (north, center and south) are well represented by a combination of a non-equilibrium ionization (PSHOCK) and a power-law (PL) model. The mid-infrared observations show a bright filamentary structure along the north-south direction coincident with the NW radio shell. This suggests that Kes 17 is propagating in a non-uniform environment with high density and that the shock front is interacting with several adjacent massive molecular clouds. The good correspondence of radio and mid-infrared emissions suggests that the filamentary features are caused by shock compression. The X-ray characteristics and well-known radio parameters indicate that G304.6+0.1 is a middle-aged SNR (2.8−6.4) × 104 yr old and a new member of the recently proposed group of mixed-morphology SNRs. |
description |
Fil: Combi, Jorge A. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico la Plata. Instituto Argentino de Radioastronomia (i); Argentina. |
publishDate |
2010 |
dc.date.none.fl_str_mv |
2010-09-13 |
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 |
Combi, Jorge A., Albacete Colombo, Juan F., Sánchez Ayaso, Estrella, Romero, Gustavo E., Marti, J. (2010). XMM-Newton detection of the supernova remnant G304.6+0.1 (Kes 17); Edp Sciences; Astronomy And Astrophysics 1432-0746 0004-6361 https://www.aanda.org/articles/aa/abs/2010/15/aa13935-09/aa13935-09.html https://rid.unrn.edu.ar/jspui/handle/20.500.12049/2507 http://dx.doi.org/10.1051/0004-6361/200913935 http://hdl.handle.net/11336/18905 |
identifier_str_mv |
Combi, Jorge A., Albacete Colombo, Juan F., Sánchez Ayaso, Estrella, Romero, Gustavo E., Marti, J. (2010). XMM-Newton detection of the supernova remnant G304.6+0.1 (Kes 17); Edp Sciences; Astronomy And Astrophysics 1432-0746 0004-6361 |
url |
https://www.aanda.org/articles/aa/abs/2010/15/aa13935-09/aa13935-09.html https://rid.unrn.edu.ar/jspui/handle/20.500.12049/2507 http://dx.doi.org/10.1051/0004-6361/200913935 http://hdl.handle.net/11336/18905 |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
523 Astronomy And Astrophysics |
dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by-nc-sa/4.0/ |
eu_rights_str_mv |
openAccess |
rights_invalid_str_mv |
https://creativecommons.org/licenses/by-nc-sa/4.0/ |
dc.format.none.fl_str_mv |
application/pdf |
dc.publisher.none.fl_str_mv |
Edp Sciences |
publisher.none.fl_str_mv |
Edp Sciences |
dc.source.none.fl_str_mv |
reponame:RID-UNRN (UNRN) instname:Universidad Nacional de Río Negro |
reponame_str |
RID-UNRN (UNRN) |
collection |
RID-UNRN (UNRN) |
instname_str |
Universidad Nacional de Río Negro |
repository.name.fl_str_mv |
RID-UNRN (UNRN) - Universidad Nacional de Río Negro |
repository.mail.fl_str_mv |
rid@unrn.edu.ar |
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12.982451 |