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| Campo DC | Valor | Lengua/Idioma |
|---|---|---|
| dc.contributor.author | Combi, Jorge A. | - |
| dc.contributor.author | Albacete Colombo, Juan Facundo | - |
| dc.contributor.author | Sánchez Ayaso, Estrella | - |
| dc.contributor.author | Romero, Gustavo E. | - |
| dc.contributor.author | Marti, J. | - |
| dc.contributor.author | Luque Escamilla, P. L. | - |
| dc.contributor.author | Muñoz Arjonilla, A. J. | - |
| dc.contributor.author | Sánchez Sutil, J. R. | - |
| dc.contributor.author | López Santiago, J. | - |
| dc.date.accessioned | 2019-07-03T13:09:12Z | - |
| dc.date.available | 2019-07-03T13:09:12Z | - |
| dc.date.issued | 2010-09-13 | - |
| dc.identifier.citation | 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 | es_ES |
| dc.identifier.issn | 1432-0746 | es_ES |
| dc.identifier.issn | 0004-6361 | es_ES |
| dc.identifier.uri | https://www.aanda.org/articles/aa/abs/2010/15/aa13935-09/aa13935-09.html | - |
| dc.identifier.uri | https://rid.unrn.edu.ar/jspui/handle/20.500.12049/2507 | - |
| dc.format.extent | P. 76-80 | es_ES |
| dc.format.medium | impreso | es_ES |
| dc.format.medium | digital | es_ES |
| dc.language.iso | en | es_ES |
| dc.publisher | Edp Sciences | es_ES |
| dc.title | XMM-Newton detection of the supernova remnant G304.6+0.1 (Kes 17) | es_ES |
| dc.type | Articulo | es_ES |
| dc.rights.license | https://creativecommons.org/licenses/by-nc-sa/4.0/ | es_ES |
| dc.description.filiation | Fil: Combi, Jorge A. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico la Plata. Instituto Argentino de Radioastronomia (i); Argentina. | es_ES |
| dc.description.filiation | Fil: Combi, Jorge A. Universidad de Jaén; España | es_ES |
| dc.description.filiation | Fil: Combi, Jorge A. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina | es_ES |
| dc.description.filiation | Fil: Albacete Colombo, Juan F. Universidad Nacional del Comahue; Argentina | es_ES |
| dc.description.filiation | Fil: Sánchez Ayaso, Estrella. Universidad de Jaén; España | es_ES |
| dc.description.filiation | 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 | es_ES |
| dc.description.filiation | Fil: Romero, Gustavo E. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina | es_ES |
| dc.description.filiation | Fil: Marti, J. Universidad de Jaén; España | es_ES |
| dc.description.filiation | Fil: Luque Escamilla, P. L. Escuela Politécnica Superior, Universidad de Jaén. Departamento de Ingeniería Mecánica y Minera; España | es_ES |
| dc.description.filiation | Fil: Muñoz Arjonilla, A. J. Escuela Politécnica Superior, Universidad de Jaén. Departamento de Ingeniería Mecánica y Minera; España | es_ES |
| dc.description.filiation | Fil: Sánchez Sutil, J. R. Escuela Politécnica Superior, Universidad de Jaén. Departamento de Ingeniería Mecánica y Minera; España | es_ES |
| dc.description.filiation | Fil: López Santiago, J. Universidad Complutense de Madrid. Departamento de Astrofísica y Ciencias de la Atmósfera; España | es_ES |
| dc.subject.keyword | ISM: Individual Objects: G304.6+0.1 | es_ES |
| dc.subject.keyword | ISM: Supernova Remnants | es_ES |
| dc.subject.keyword | X-rays: ISM | es_ES |
| dc.subject.keyword | Radiation Mechanisms: Thermal | es_ES |
| dc.type.version | info:eu-repo/semantics/publishedVersion | es_ES |
| dc.subject.materia | Ciencias Exactas y Naturales | es_ES |
| dc.origin.lugarDesarrollo | Universidad Nacional de Río Negro | es_ES |
| dc.relation.journalissue | 523 | es_ES |
| dc.description.review | true | es_ES |
| dc.description.resumen | 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. | es_ES |
| dc.identifier.doi | http://dx.doi.org/10.1051/0004-6361/200913935 | - |
| dc.identifier.handle | http://hdl.handle.net/11336/18905 | - |
| dc.relation.journalTitle | Astronomy And Astrophysics | es_ES |
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