Observational constraints on energetic particle diffusion in young supernovae remnants: Amplified magnetic field and maximum energy

Astronomy and Astrophysics

Volumn 453, Issue 2, 2006, Pages 387-395

  Parizot, E ^a   Marcowith, A ^b   Ballet, J ^c   Gallant, Y A ^d  

^a CNRS   (France)

^b IRAP   (France)

^c CEA SACLAY   (France)

^d CENTRE DE CALCUL DE L INSTITUT NATIONAL DE PHYSIQUE NUCLEAIRE ET DE PHYSIQUE DES PARTICULES   (France)

Author keywords

Acceleration of particles; Cosmic rays; ISM: supernova remnants; Magnetic fields

Indexed keywords

CONSTRAINT THEORY; COSMIC RAYS; DIFFUSION; IRON; MAGNETIC FIELDS; PROTONS;

ACCELERATION OF PARTICLES; BOHM DIFFUSION; COSMIC-RAY SPECTRUM; ISM: SUPERNOVA REMNANTS;

ASTROPHYSICS;

EID: 33745752569     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20064985     Document Type: Article

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