The high energy gamma-ray emission expected from Tycho's supernova remnant

Astronomy and Astrophysics

Volumn 396, Issue 2, 2002, Pages 649-656

  Völk, Heinrich J ^a   Berezhko, E G ^b   Ksenofontov, L T ^b   Rowell, Gavin P ^a  

^a MAX PLANCK INSTITUT FÜR KERNPHYSIK   (Germany)

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

Author keywords

Acceleration of particles; Gamma rays: theory; Radiation mechanisms: non thermal; Radio continuum: ISM; Stars: supernovae: individual: Tycho's SNR; X rays: ISM

Indexed keywords

COSMIC RAYS; EMISSION SPECTROSCOPY; GAMMA RAYS; MAGNETIC FIELDS; MICROWAVES; NONLINEAR SYSTEMS; PARTICLE ACCELERATORS; RADIO WAVES; X RAYS;

NONLINEAR KINETIC MODELS;

ASTROPHYSICS;

EID: 0036903496     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20021407     Document Type: Article

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