Constraints on cosmic-ray origin from TeV gamma-ray observations of supernova remnants

If supernova remnants (SNRs) are the site of cosmicray acceleration, the associated nuclear interactions should result in an observable flux of γ-rays for the nearest SNRs. Measurements of the TeV γ-ray flux from six nearby, radio-bright SNRs have been made with the Whipple Observatory imaging air Č...

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Detalles Bibliográficos
Publicado:	1998
Materias:	Cosmic rays Gamma-rays: observations ISM: IC 443; γ Cyg SNR; W 44 SNRS
Acceso en línea:	https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00046361_v329_n2_p639_Buckley http://hdl.handle.net/20.500.12110/paper_00046361_v329_n2_p639_Buckley
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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