Morphological evidence for azimuthal variations of the cosmic-ray ion acceleration at the blast wave of SN 1006
Using radio, X-ray, and optical observations, we present evidence for morphological changes due to efficient cosmic ray ion acceleration in the structure of the southeastern region of the supernova remnant SN 1006. SN 1006 has an apparent bipolar morphology in both the radio and high-energy X-ray sy...
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| Autores principales: | Cassam-Chenai, G., Hughes, J.P., Reynoso, E.M., Badenes, C., Moffett, D. |
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| Formato: | Artículo publishedVersion |
| Publicado: |
2008
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| Materias: | |
| Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_0004637X_v680_n2_p1180_CassamChenai https://repositoriouba.sisbi.uba.ar/gsdl/cgi-bin/library.cgi?a=d&c=artiaex&d=paper_0004637X_v680_n2_p1180_CassamChenai_oai |
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