Strong evidence for hadron acceleration in Tycho's supernova remnant

Astronomy and Astrophysics

Volumn 538, Issue , 2012, Pages

  Morlino, G ^a   Caprioli, D ^a  

^a INAF OSSERVATORIO ASTROFISICO DI ARCETRI   (Italy)

Author keywords

Cosmic rays; ISM: supernova remnants; Radiation mechanisms: non thermal; Shock waves

Indexed keywords

ACCELERATED PARTICLES; BACK REACTION; BACKGROUND GAS; COMPRESSION FACTOR; DIFFUSIVE SHOCK ACCELERATIONS; ENERGY SPECTRA; FERMI MECHANISM; FIRST-ORDER; GAMMA RAY SPECTRA; GAMMA-RAY EMISSION; GAMMA-RAY OBSERVATIONS; INVERSE COMPTON SCATTERING; ISM: SUPERNOVA REMNANTS; MAGNETIC FIELD AMPLIFICATION; MAGNETIC TURBULENCE; MULTIWAVELENGTH; N-WAVES; NEUTRAL PIONS; NONTHERMAL EMISSION; NUCLEAR COLLISIONS; PARTICLE ACCELERATION; RADIATION MECHANISMS: NON-THERMAL; RELATIVISTIC ELECTRON; SELF-CONSISTENCY; SEMI-ANALYTICAL; STRONG MAGNETIC FIELDS; SUPERNOVA REMNANTS; TYCHO'S SUPERNOVA REMNANT; VERITAS;

AMPLIFICATION; COSMIC RAYS; GAMMA RAYS; HADRONS; MAGNETIC FIELDS; PARTICLE ACCELERATORS; SHOCK WAVES; TELLURIUM COMPOUNDS; ULTRAVIOLET SPECTROSCOPY;

STARS;

EID: 84856736598     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201117855     Document Type: Article

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