Diffusive synchrotron radiation from pulsar wind nebulae

Monthly Notices of the Royal Astronomical Society

Volumn 376, Issue 2, 2007, Pages 625-633

  Fleishman, G D ^a,b   Bietenholz, M F ^c  

^a NATIONAL RADIO ASTRONOMY OBSERVATORY   (United States)

^b IOFFE INSTITUTE   (Russian Federation)

^c YORK UNIVERSITY   (Canada)

Author keywords

Acceleration of particles; Magnetic fields; Radiation mechanisms: non thermal; Shock waves; Supernova remnants; Turbulence

Indexed keywords

CHARGED PARTICLES; COSMOLOGY; EMISSION SPECTROSCOPY; GALAXIES; MAGNETIC FIELDS; SHOCK WAVES; STOCHASTIC SYSTEMS; SYNCHROTRONS;

ACCELERATION OF PARTICLES; MAGNETIC-FIELD; PARTICLE TRAJECTORIES; PULSAR WIND NEBULA; RADIATION MECHANISMS: NONTHERMAL; RANDOM WALK; SHOCK-WAVES; SPECTRA'S; STOCHASTIC MAGNETIC FIELD; SUPERNOVA REMNANTS;

SYNCHROTRON RADIATION;

EID: 34247244249     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2007.11450.x     Document Type: Article

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