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Campo DC | Valor | Lengua/Idioma |
---|---|---|
dc.provenance | Universidad Nacional de Río Negro | - |
dc.creator | Combi, Jorge A. | - |
dc.creator | Albacete Colombo, Juan F. | - |
dc.creator | Romero, Gustavo E. | - |
dc.creator | Benaglia, Paula | - |
dc.date | 2007-06 | - |
dc.date.accessioned | 2020-02-11T14:08:30Z | - |
dc.date.available | 2020-02-11T14:08:30Z | - |
dc.date.issued | 2007-06 | - |
dc.identifier | Combi, Jorge A., Albacete Colombo, Juan F., Romero, Gustavo E. Benaglia, Paula. (2007). Hard X-ray emission from the SNR G337.2+0.1; Springer; Astrophysics And Space Science. | - |
dc.identifier | 0004-640 | - |
dc.identifier | 1572-946 | - |
dc.identifier | https://link.springer.com/article/10.1007%2Fs10509-007-9426-7 | - |
dc.identifier | https://rid.unrn.edu.ar/jspui/handle/20.500.12049/2501 | - |
dc.identifier | http://dx.doi.org/10.1007/s10509-007-9426-7 | - |
dc.identifier | http://hdl.handle.net/11336/27801 | - |
dc.identifier.uri | http://rodna.bn.gov.ar/jspui/handle/bnmm/575678 | - |
dc.description | Fil: Combi, Jorge A. Universidad de Jaén; España. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina | - |
dc.description | Fil: Albacete Colombo, Juan F. Istituto Nazionale Di Astrofísica. Osservatorio Astronómico Di Palermo; Italia. | - |
dc.description | Fil: Albacete Colombo, Juan F. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina | - |
dc.description | Fil: Romero, Gustavo E. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina | - |
dc.description | Fil: Benaglia, Paula. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina | - |
dc.description | We report the hard X-ray emission of the SNR candidate G337.2+0.1. The object shows centrally filled and diffuse X-ray emission, which peaks in the hard 3.0−10.0 keV band. A spectral study confirms that the column density of the central part of the object is about NH ∼5.9(±1.5)×1022 cm−2 and its X-ray spectrum is well represented by a single power-law with a photon index Γ=0.96±0.56. Detailed spectral analysis indicates that the outer region is highly absorbed and quite softer than the inner region. Such characteristics are already observed in other X-ray plerions. Based on the morphological and spectral X-ray information, we confirm the SNR nature of G337.2+0.1, and suggest that the central region of the source is a pulsar wind nebula (PWN), originated by an energetic though yet undetected pulsar, that is currently losing energy at a rate of ∼ 1036 erg s−1 . | - |
dc.format | application/pdf | - |
dc.language | eng | - |
dc.publisher | Springer | - |
dc.relation | 309 | - |
dc.relation | Astrophysics And Space Science | - |
dc.rights | info:eu-repo/semantics/openAccess | - |
dc.rights | https://creativecommons.org/licenses/by-nc-sa/4.0/ | - |
dc.source | reponame:RID-UNRN (UNRN) | - |
dc.source | instname:Universidad Nacional de Río Negro | - |
dc.source | instacron:UNRN | - |
dc.source.uri | http://hdl.handle.net/11336/27801 | - |
dc.subject | Supernova Remnants | - |
dc.subject | X-Rays | - |
dc.subject | AX J1635.9−4719 (Remanente de Supernova) | - |
dc.subject | G337.2+0.1 (Estrella) | - |
dc.subject | Interstellar Medium | - |
dc.subject | Radiation Mechanisms | - |
dc.subject | Non Thermal Mechanisms | - |
dc.subject | .::Ciencias Exactas y Naturales | - |
dc.title | Hard X-ray emission from the SNR G337.2+0.1 | - |
dc.type | info:eu-repo/semantics/article | - |
dc.type | info:eu-repo/semantics/publishedVersion | - |
dc.type | info:ar-repo/semantics/articulo | - |
dc.about | - | |
Aparece en las colecciones: | Universidad Nacional de Río Negro |
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