Artículo
Schneiter, E.M.; Velázquez, P.F.; Reynoso, E.M.; Esquivel, A.; De Colle, F. "3D MHD simulation of polarized emission in SN 1006" (2015) Monthly Notices of the Royal Astronomical Society. 449(1):88-93
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Abstract:
We use three-dimensional magnetohydrodynamic simulations to model the supernova remnant SN 1006. From our numerical results, we have carried out a polarization study, obtaining synthetic maps of the polarized intensity, the Stokes parameter Q, and the polar-referenced angle, which can be compared with observational results. Synthetic maps were computed considering two possible particle acceleration mechanisms: quasi-parallel and quasi-perpendicular. The comparison of synthetic maps of the Stokes parameter Q maps with observations proves to be a valuable tool to discern unambiguously which mechanism is taking place in the remnant of SN 1006, giving strong support to the quasi-parallel model. © 2015 The Authors.
Registro:
| Documento: | Artículo |
| Título: | 3D MHD simulation of polarized emission in SN 1006 |
| Autor: | Schneiter, E.M.; Velázquez, P.F.; Reynoso, E.M.; Esquivel, A.; De Colle, F. |
| Filiación: | Instituto de Astronomía Téorica y Experimental, Universidad Nacional de Córdoba, Córdoba, X5000BGR, Argentina Departamento de Materiales y Tecnologia, UNC, Córdoba, X5000JKP, Argentina Deparment of Astronomy, Oskar Klein Centre, Albanova, Stockholm University, Stockholm, SE-106 91, Sweden Instituto de Ciencias Nucleares, Universidad Nacional de MexicoDF 04510, Mexico Instituto de Astronomía y Física del Espacio, Suc. 28, CP: 1428, Buenos Aires, Argentina Physics Department, Faculty of Exact and Natural Sciences, University of Buenos AiresC1428EHA, Argentina |
| Palabras clave: | ISM: supernova remnants; Methods: numerical; MHD; Radiation mechanisms: general; Supernovae: individual: SN 1006 |
| Año: | 2015 |
| Volumen: | 449 |
| Número: | 1 |
| Página de inicio: | 88 |
| Página de fin: | 93 |
| DOI: | http://dx.doi.org/10.1093/mnras/stv279 |
| Título revista: | Monthly Notices of the Royal Astronomical Society |
| Título revista abreviado: | Mon. Not. R. Astron. Soc. |
| ISSN: | 00358711 |
| CODEN: | MNRAA |
| Registro: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00358711_v449_n1_p88_Schneiter |
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Citas:
---------- APA ----------
Schneiter, E.M., Velázquez, P.F., Reynoso, E.M., Esquivel, A. & De Colle, F. (2015) . 3D MHD simulation of polarized emission in SN 1006. Monthly Notices of the Royal Astronomical Society, 449(1), 88-93.http://dx.doi.org/10.1093/mnras/stv279
---------- CHICAGO ----------
Schneiter, E.M., Velázquez, P.F., Reynoso, E.M., Esquivel, A., De Colle, F. "3D MHD simulation of polarized emission in SN 1006" . Monthly Notices of the Royal Astronomical Society 449, no. 1 (2015) : 88-93.http://dx.doi.org/10.1093/mnras/stv279
---------- MLA ----------
Schneiter, E.M., Velázquez, P.F., Reynoso, E.M., Esquivel, A., De Colle, F. "3D MHD simulation of polarized emission in SN 1006" . Monthly Notices of the Royal Astronomical Society, vol. 449, no. 1, 2015, pp. 88-93.http://dx.doi.org/10.1093/mnras/stv279
---------- VANCOUVER ----------
Schneiter, E.M., Velázquez, P.F., Reynoso, E.M., Esquivel, A., De Colle, F. 3D MHD simulation of polarized emission in SN 1006. Mon. Not. R. Astron. Soc. 2015;449(1):88-93.http://dx.doi.org/10.1093/mnras/stv279
