Geometry of the non-thermal emission in SN 1006: Azlmuthal variations of cosmic-ray acceleration

SN 1006 is the prototype of shell supernova remnants, in which non-thermal synchrotron emission dominates the X-ray spectrum. The non-thermal emission is due to the cosmic-ray electrons accelerated behind the blast wave. The X-ray synchrotron emission is due to the highest energy electrons, and is t...

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Detalles Bibliográficos
Autores principales:	Rothenflug, R., Ballet, J., Dubner, G., Giacani, E., Decourchelle, A., Ferrando, P.
Formato:	JOUR
Materias:	Acceleration of particles ISM: cosmic rays ISM: supernova remnants Magnetic fields X-rays: individuals: SN 1006 Data reduction Fourier transforms Galaxies Interferometers Magnetic field effects Mathematical models Polynomials Synchrotrons X rays ISM:cosmic rays ISM:supernova remnants X-rays:individuals:SN 1006 Cosmic rays
Acceso en línea:	http://hdl.handle.net/20.500.12110/paper_00046361_v425_n1_p121_Rothenflug
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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