Erratum: Constraining the population of cosmic ray protons in cooling flow clusters with γ-ray and radio observations: Are radio mini-halos of hadronic origin? (Astronomy and Astrophysics (2004) 413 (17-36) DOI: 10.1051/0004-6361:20031464);Constraining the population of cosmic ray protons in cooling flow clusters with γ-ray and radio observations: Are radio mini-halos of hadronic origin?

Astronomy and Astrophysics

Volumn 413, Issue 1, 2004, Pages 17-36

  Pfrommer, C ^a   Ensslin T A ^a  

^a MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

Author keywords

Galaxies: cluster: general; Galaxies: cluster: individual: Perseus (A426); Galaxies: cooling flows; Galaxies: intergalactic medium; ISM: cosmic rays; Radiation mechanisms: non thermal; Errata, addenda; Galaxies: clusters: general; Galaxies: clusters: individual: Perseus (A426)

Indexed keywords

COMPUTER SIMULATION; COOLING; COSMIC RAYS; GALAXIES; GAMMA RAYS; MAGNETIC FIELDS; MATHEMATICAL MODELS; PHOTONS; SYNCHROTRONS;

HADRONIC INTERACTIONS; MAGNETIC ENERGY DENSITIES; RADIO FLUX; SYNCHROTRON EMISSION;

ASTROPHYSICS;

EID: 0347540928     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20041826     Document Type: Erratum

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