Gamma-ray emission expected from Kepler's supernova remnant

Astronomy and Astrophysics

Volumn 452, Issue 1, 2006, Pages 217-221

  Berezhko, E G ^a   Ksenofontov, L T ^a   Volk H J ^b  

^a YU G SHAFER INSTITUTE OF COSMOPHYSICAL RESEARCH AND AERONOMY   (Russian Federation)

^b MAX PLANCK INSTITUT FÜR KERNPHYSIK   (Germany)

Author keywords

Acceleration of particles; Cosmic rays; Gamma rays: theory; Hydrodynamics; ISM: supernova remnants; Radiation mechanisms: non thermal

Indexed keywords

COSMIC RAYS; EMISSION SPECTROSCOPY; GAMMA RAYS; HYDRODYNAMICS; KINETIC THEORY; MAGNETIC FLUX; PARAMETER ESTIMATION; REMANENCE; SPACE RESEARCH; SPECTRUM ANALYSIS;

ACCELERATION OF PARTICLES; GAMMA RAYS: THEORY; INTERSTELLAR MEDIUM (ISM); ISM: SUPERNOVA REMNANTS; RADIATION MECHANISMS: NON-THERMAL;

GALAXIES;

EID: 33744952667     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20064801     Document Type: Article

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