Modeling the shock-cloud interaction in SN 1006: Unveiling the origin of nonthermal X-ray and γ-ray emission

Context. The supernova remnant SN 1006 is a source of high-energy particles and its southwestern limb is interacting with a dense ambient cloud, thus is a promising region for γ-ray hadronic emission. Aims. We aim at describing the physics and the nonthermal emission associated with the shock-cloud...

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Detalles Bibliográficos
Autores principales:	Miceli, M., Orlando, S., Pereira, V., Acero, F., Katsuda, S., Decourchelle, A., Winkler, F.P., Bonito, R., Reale, F., Peres, G., Li, J., Dubner, G.
Formato:	JOUR
Materias:	Acceleration of particles ISM: clouds ISM: individual objects: SN 1006 ISM: supernova remnants Magnetohydrodynamics (MHD) X-rays: ISM Cutoff frequency Magnetohydrodynamics Supernovae Synchrotron radiation ISM : clouds Ism: individual objects: sn 1006 X rays: ISM Gamma rays
Acceso en línea:	http://hdl.handle.net/20.500.12110/paper_00046361_v593_n_p_Miceli
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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