Morphological evidence for azimuthal variations of the cosmic-ray ion acceleration at the blast wave of SN 1006

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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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Detalles Bibliográficos
Autores principales: Cassam-Chenai, G., Hughes, J.P., Reynoso, E.M., Badenes, C., Moffett, D.
Formato: JOUR
Materias:
Acceleration of particles
Cosmic rays
ISM: individual (SN 1006)
Shock waves
Supernova remnants
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_0004637X_v680_n2_p1180_CassamChenai
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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