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...
Guardado en:
| Publicado: |
2017
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| Acceso en línea: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00358711_v472_n2_p2117_MoranchelBasurto http://hdl.handle.net/20.500.12110/paper_00358711_v472_n2_p2117_MoranchelBasurto |
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