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
Autores principales: Buckley, J.H., Akerlof, C.W., Carter-Lewis, D.A., Catanese, M., Cawley, M.F., Connaughton, V., Fegan, D.J., Finley, J.P., Gaidos, J.A., Hillas, A.M., Krennrich, F., Lamb, R.C., Lessard, R.W., McEnery, J.E., Mohanty, G., Quinn, J., Rodgers, A.J., Rose, H.J., Rovero, A.C., Schubnell, M.S., Sembroski, G., Srinivasan, R., Weekes, T.C., Zweerink, J.
Formato: JOUR
Materias:
Cosmic rays
Gamma-rays: observations
ISM: IC 443; γ Cyg SNR; W 44
SNRS
Acceso en línea: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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