A statistical approach to radio emission from shell-type SNRs-I. Basic ideas, techniques, and first results

Astronomy and Astrophysics

Volumn 509, Issue 1, 2010, Pages

  Bandiera, R ^a   Petruk, O ^b  

^a INAF OSSERVATORIO ASTROFISICO DI ARCETRI   (Italy)

^b PIDSTRYHACH INSTITUTE FOR APPLIED PROBLEMS OF MECHANICS AND MATHEMATICS   (Ukraine)

Author keywords

Individual; ISM; M 33 Galaxies; M 82; Non thermal Acceleration of particles Galaxies; Statistical Radiation mechanisms; Supernova remnants Methods

Indexed keywords

AMPLIFICATION; MAGNETIC FIELDS; PARTICLE ACCELERATOR ACCESSORIES; SIGNAL TO NOISE RATIO; SYNCHROTRON RADIATION; SYNCHROTRONS;

ACCELERATION OF PARTICLES; INDIVIDUAL; ISM; NONTHERMAL; RADIATION MECHANISM; SUPERNOVA REMNANTS;

GALAXIES;

EID: 76349109250     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200912244     Document Type: Article

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