Aspect angle for interstellar magnetic field in SN 1006

Monthly Notices of the Royal Astronomical Society

Volumn 393, Issue 3, 2009, Pages 1034-1040

  Petruk, O ^a,b   Dubner, G ^c   Castelletti, G ^c   Bocchino, F ^d,e   Iakubovskyi, D ^f   Kirsch, M G F ^g   Miceli, M ^d,e   Orlando, S ^d,e   Telezhinsky, I ^h  

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

^b IVAN FRANKO NATIONAL UNIVERSITY OF LVIV   (Ukraine)

^c INSTITUTO DE ASTRONOMÍA Y FÍSICA DEL ESPACIO   (Argentina)

^d INAF OSSERVATORIO ASTROFISICO DI TORINO   (Italy)

^e Consorzio COMETA ^*  (Italy)

^f BOGOLYUBOV INSTITUTE FOR THEORETICAL PHYSICS   (Ukraine)

^g ESA ESOC   (Germany)

^h TARAS SHEVCHENKO NATIONAL UNIVERSITY OF KYIV   (Ukraine)

Author keywords

Acceleration of particles; Cosmic rays; ISM: individual: SN 1006; Radiation mechanisms: non thermal; Shock waves; Supernova remnants

Indexed keywords

COSMIC RAYS; COSMOLOGY; EFFICIENCY; MAGNETIC FIELDS; SUPERNOVAE;

ACCELERATION OF PARTICLES; ASPECTS ANGLE; INJECTION EFFICIENCY; INTERSTELLAR MAGNETIC FIELDS; ISM: INDIVIDUAL: SN 1006; ISM: INDIVIDUALS; LINE OF SIGHT; RADIATION MECHANISMS: NONTHERMAL; SHOCK-WAVES; SUPERNOVA REMNANTS;

SHOCK WAVES;

EID: 60349118508     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2008.14251.x     Document Type: Article

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