Magnetic fields in supernova remnants and pulsar-wind nebulae

Space Science Reviews

Volumn 166, Issue 1-4, 2012, Pages 231-261

  Reynolds, Stephen P ^a   Gaensler, B M ^b   Bocchino, Fabrizio ^c  

^a NORTH CAROLINA STATE UNIVERSITY   (United States)

^b UNIVERSITY OF SYDNEY   (Australia)

^c INAF OSSERVATORIO ASTRONOMICO DI PALERMO   (Italy)

Author keywords

Magnetic field amplification; Pulsar wind nebulae; Supernova remnants

Indexed keywords

COSMIC MICROWAVE BACKGROUNDS; DEGREE OF ORDER; DENSITY GRADIENTS; DYNAMICAL MODELING; ELECTRON ACCELERATION; EMISSION PROCESS; EQUIPARTITION; IN-SHELL; LOWER LIMITS; MAGNETIC FIELD STRENGTHS; MAGNETIC-FIELD GEOMETRY; MHD MODELS; ORDERS OF MAGNITUDE; PULSAR-WIND NEBULAE; RADIATIVE LOSS; RADIO EMISSION; SPATIAL ANALYSIS; SUPERNOVA REMNANTS; SYNCHROTRON X RAYS; TIME-SCALES; TOROIDAL STRUCTURES; UPPER LIMITS;

ELECTROMAGNETIC WAVE EMISSION; GALAXIES; GAMMA RAYS; STARS; TELLURIUM COMPOUNDS; X RAY SCATTERING;

MAGNETIC FIELDS;

EID: 84860769404     PISSN: 00386308     EISSN: 15729672     Source Type: Journal    
DOI: 10.1007/s11214-011-9775-y     Document Type: Review

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