Constraints on the diffusive shock acceleration from the nonthermal X-ray thin shells in SN 1006 NE rim

Astronomy and Astrophysics

Volumn 416, Issue 2, 2004, Pages 595-602

  Yamazaki, R ^a   Yoshida, T ^b   Terasawa, T ^c   Bamba, A ^a   Koyama, K ^a  

^a KYOTO UNIVERSITY   (Japan)

^b IBARAKI UNIVERSITY   (Japan)

^c UNIVERSITY OF TOKYO   (Japan)

Author keywords

Acceleration of particles; ISM: supernova remnants; X rays: individual: SN 1006

Indexed keywords

ACCELERATION; APPROXIMATION THEORY; COSMIC RAYS; DATA REDUCTION; DIFFUSION; ENERGY DISSIPATION; ESTIMATION; MAGNETIC FIELD EFFECTS; MATHEMATICAL MODELS; POLARIZATION; SYNCHROTRONS;

ACCELERATION OF PARTICLES; ISM:SUPERNOVA REMNANTS; X-RAYS:INDVIDUAL:SN 1006;

ASTRONOMY;

EID: 1642410283     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20034212     Document Type: Article

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