Evidence for particle acceleration to the knee of the cosmic ray spectrum in Tycho's supernova remnant
Supernova remnants (SNRs) have long been assumed to be the source of cosmic rays (CRs) up to the "knee" of the CR spectrum at 1015 eV, accelerating particles to relativistic energies in their blast waves by the process of diffusive shock acceleration (DSA). Since CR nuclei do not radiate e...
Guardado en:
Autores principales: | Eriksen, K.A., Hughes, J.P., Badenes, C., Fesen, R., Ghavamian, P., Moffett, D., Plucinksy, P.P., Rakowski, C.E., Reynoso, E.M., Slane, P. |
---|---|
Formato: | JOUR |
Materias: | |
Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_20418205_v728_n2PARTII_p_Eriksen |
Aporte de: |
Ejemplares similares
-
Evidence for particle acceleration to the knee of the cosmic ray spectrum in Tycho's supernova remnant
Publicado: (2011) -
Cosmic-ray acceleration at the forward shock in Tycho's supernova remnant: Evidence from Chandra X-ray observations
por: Warren, J.S., et al. -
A vla study of the expansion of tycho's supernova remnant
por: Reynoso, E.M., et al. -
Study of the Rayleigh-Taylor instability in Tycho's supernova remnant
por: Velázquez, P.F., et al. -
Study of the Rayleigh-Taylor instability in Tycho's supernova remnant
Publicado: (1998)