Polarisation properties of Milky-Way-like galaxies

Astronomy and Astrophysics

Volumn 543, Issue , 2012, Pages

  Sun, X H ^a,b,c   Reich, W ^a  

^a MAX PLANCK INSTITUT FÜR RADIOASTRONOMIE   (Germany)

^b UNIVERSITY OF SYDNEY   (Australia)

^c CHINESE ACADEMY OF SCIENCES   (China)

Author keywords

ISM: magnetic fields; Polarization; Radio continuum: general

Indexed keywords

CURRENT ANALYSIS; EMISSION MODEL; ENERGY EQUIPARTITION; HIGH FREQUENCY HF; INCLINATION ANGLES; ISM: MAGNETIC FIELDS; K FACTOR; MAGNETIC FIELD STRENGTHS; MILKY WAY GALAXY; MILKY WAYS; MODEL PARAMETERS; NUMBER DISTRIBUTION; POSITION ANGLE; RADIO CONTINUUM: GENERAL; SPIRAL GALAXIES; SYNCHROTRON EMISSION; TECHNIQUES USED;

MAGNETIC FIELDS; POLARIZATION; SYNCHROTRON RADIATION; THREE DIMENSIONAL;

GALAXIES;

EID: 84863730930     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201218802     Document Type: Article

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