Cosmic-ray driven dynamo in the interstellar medium of irregular galaxies

Astronomy and Astrophysics

Volumn 510, Issue 1, 2010, Pages

  Siejkowski, H ^a   Soida, M ^a   Otmianowska Mazur, K ^a   Hanasz, M ^b   Bomans, D J ^c  

^a JAGIELLONIAN UNIVERSITY   (Poland)

^b NICOLAUS COPERNICUS UNIVERSITY   (Poland)

^c RUHR UNIVERSITY BOCHUM   (Germany)

Author keywords

Galaxies: irregular; ISM: magnetic fields; Magnetohydrodynamics (MHD); Methods: numerical

Indexed keywords

DIFFERENTIAL ROTATION; ESSENTIAL ELEMENTS; GALAXIES: IRREGULAR; INTERSTELLAR MEDIUMS; ISM: MAGNETIC FIELDS; ITS EFFICIENCIES; MAGNETIC ENERGIES; MAGNETIC RECONNECTIONS; MAGNETOHYDRODYNAMICS (MHD); METHODS: NUMERICAL; NUMERICAL MODELS; RADIO OBSERVATION; RAY-DRIVEN; SHEARING RATES; SIMULATION BOXES; SLOW ROTATION; SPIRAL GALAXIES; STAR FORMATIONS;

COSMIC RAYS; COSMOLOGY; ELECTRIC GENERATORS; GALAXIES; INTERACTIVE DEVICES; MAGNETIC FIELDS; NUMERICAL METHODS; ROTATION; SHEARING;

MAGNETOHYDRODYNAMICS;

EID: 79952858450     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200912729     Document Type: Article

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