Origin of the bilateral structure of the supernova remnant G296.5+10
In this work, we have modelled the supernova remnant (SNR) G296.5+10, by means of 3D magnetohydrodynamics (MHD) simulations. This remnant belongs to the bilateral SNR group and has an additional striking feature: the rotation measure (RM) in its eastern and western parts are very different. In order...
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Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_00358711_v472_n2_p2117_MoranchelBasurto |
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todo:paper_00358711_v472_n2_p2117_MoranchelBasurto2023-10-03T14:47:21Z Origin of the bilateral structure of the supernova remnant G296.5+10 Moranchel-Basurto, A. Velázquez, P.F. Giacani, E. Toledo-Roy, J.C. Schneiter, E.M. De Colle, F. Esquivel, A. ISM: supernova remnants Methods: numerical MHD Radiation mechanisms: non-thermal Shock waves In this work, we have modelled the supernova remnant (SNR) G296.5+10, by means of 3D magnetohydrodynamics (MHD) simulations. This remnant belongs to the bilateral SNR group and has an additional striking feature: the rotation measure (RM) in its eastern and western parts are very different. In order to explain both the morphology observed in radio-continuum and the RM, we consider that the remnant expands into a medium shaped by the superposition of the magnetic field of the progenitor star with a constant Galactic magnetic field. We have also carried out a polarization study from our MHD results, obtaining synthetic maps of the linearly polarized intensity and the Stokes parameters. This study reveals that both the radio morphology and the reported RM for G296.5+10 can be explained if the quasi-parallel acceleration mechanism is taking place in the shock front of this remnant. © 2017 The Authors. JOUR info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_00358711_v472_n2_p2117_MoranchelBasurto |
institution |
Universidad de Buenos Aires |
institution_str |
I-28 |
repository_str |
R-134 |
collection |
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) |
topic |
ISM: supernova remnants Methods: numerical MHD Radiation mechanisms: non-thermal Shock waves |
spellingShingle |
ISM: supernova remnants Methods: numerical MHD Radiation mechanisms: non-thermal Shock waves Moranchel-Basurto, A. Velázquez, P.F. Giacani, E. Toledo-Roy, J.C. Schneiter, E.M. De Colle, F. Esquivel, A. Origin of the bilateral structure of the supernova remnant G296.5+10 |
topic_facet |
ISM: supernova remnants Methods: numerical MHD Radiation mechanisms: non-thermal Shock waves |
description |
In this work, we have modelled the supernova remnant (SNR) G296.5+10, by means of 3D magnetohydrodynamics (MHD) simulations. This remnant belongs to the bilateral SNR group and has an additional striking feature: the rotation measure (RM) in its eastern and western parts are very different. In order to explain both the morphology observed in radio-continuum and the RM, we consider that the remnant expands into a medium shaped by the superposition of the magnetic field of the progenitor star with a constant Galactic magnetic field. We have also carried out a polarization study from our MHD results, obtaining synthetic maps of the linearly polarized intensity and the Stokes parameters. This study reveals that both the radio morphology and the reported RM for G296.5+10 can be explained if the quasi-parallel acceleration mechanism is taking place in the shock front of this remnant. © 2017 The Authors. |
format |
JOUR |
author |
Moranchel-Basurto, A. Velázquez, P.F. Giacani, E. Toledo-Roy, J.C. Schneiter, E.M. De Colle, F. Esquivel, A. |
author_facet |
Moranchel-Basurto, A. Velázquez, P.F. Giacani, E. Toledo-Roy, J.C. Schneiter, E.M. De Colle, F. Esquivel, A. |
author_sort |
Moranchel-Basurto, A. |
title |
Origin of the bilateral structure of the supernova remnant G296.5+10 |
title_short |
Origin of the bilateral structure of the supernova remnant G296.5+10 |
title_full |
Origin of the bilateral structure of the supernova remnant G296.5+10 |
title_fullStr |
Origin of the bilateral structure of the supernova remnant G296.5+10 |
title_full_unstemmed |
Origin of the bilateral structure of the supernova remnant G296.5+10 |
title_sort |
origin of the bilateral structure of the supernova remnant g296.5+10 |
url |
http://hdl.handle.net/20.500.12110/paper_00358711_v472_n2_p2117_MoranchelBasurto |
work_keys_str_mv |
AT moranchelbasurtoa originofthebilateralstructureofthesupernovaremnantg296510 AT velazquezpf originofthebilateralstructureofthesupernovaremnantg296510 AT giacanie originofthebilateralstructureofthesupernovaremnantg296510 AT toledoroyjc originofthebilateralstructureofthesupernovaremnantg296510 AT schneiterem originofthebilateralstructureofthesupernovaremnantg296510 AT decollef originofthebilateralstructureofthesupernovaremnantg296510 AT esquivela originofthebilateralstructureofthesupernovaremnantg296510 |
_version_ |
1782024207553527808 |