Constraints on the local interstellar magnetic field from non-thermal emission of SN1006

Astronomy and Astrophysics

Volumn 531, Issue , 2011, Pages

  Bocchino, F ^a   Orlando, S ^a   Miceli, M ^b   Petruk, O ^c  

^a INAF OSSERVATORIO ASTRONOMICO DI PALERMO   (Italy)

^b UNIVERSITY OF PALERMO   (Italy)

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

Author keywords

acceleration of particles; ISM: supernova remnants; shock waves

Indexed keywords

ACCELERATION OF PARTICLES; ASPECT ANGLES; CUT-OFF; ELECTRON POPULATION; FIELD STRENGTHS; GALACTIC MAGNETIC FIELDS; GALACTIC PLANE; INJECTION EFFICIENCY; INTERSTELLAR MAGNETIC FIELDS; ISM: SUPERNOVA REMNANTS; LINE OF SIGHT; LOCAL MAGNETIC FIELD; MHD SIMULATION; NONTHERMAL; NONTHERMAL EMISSION; NONUNIFORM MAGNETIC FIELDS; PARTICLE ACCELERATION; POLAR CAP; RADIO EMISSION; RADIO MAPS; SUPERNOVA REMNANTS;

EFFICIENCY; MAGNETIC FIELDS; MORPHOLOGY; PARTICLE ACCELERATOR ACCESSORIES; STARS; SYNCHROTRONS; THERMIONIC EMISSION; THREE DIMENSIONAL COMPUTER GRAPHICS;

MAGNETOHYDRODYNAMICS;

EID: 79959706240     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201016341     Document Type: Article

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