DEEP MORPHOLOGICAL and SPECTRAL STUDY of the SNR RCW 86 with FERMI-LAT

RCW 86 is a young supernova remnant (SNR) showing a shell-type structure at several wavelengths and is thought to be an efficient cosmic-ray (CR) accelerator. Earlier Fermi Large Area Telescope results reported the detection of γ-ray emission coincident with the position of RCW 86 but its origin (le...

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Detalles Bibliográficos
Autor principal:	Ajello, M.
Formato:	JOUR
Materias:	acceleration of particles cosmic rays ISM: individual objects (RCW 86)
Acceso en línea:	http://hdl.handle.net/20.500.12110/paper_0004637X_v819_n2_p_Ajello
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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