Properties of the warm magnetized ISM, as inferred from WSRT polarimetric imaging

Astronomy and Astrophysics

Volumn 427, Issue 1, 2004, Pages 169-177

  Haverkorn, M ^a,d   Katgert, P ^a   De Bruyn, A G ^b,c  

^a LEIDEN UNIVERSITY   (Netherlands)

^b ASTRON   (Netherlands)

^c UNIVERSITY OF GRONINGEN   (Netherlands)

^d HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

Author keywords

ISM: magnetic fields; ISM: structure; Magnetic fields; Polarization; Radio continuum: ISM; Techniques: polarimetric

Indexed keywords

CARRIER CONCENTRATION; GALAXIES; MAGNETIC FIELD EFFECTS; MAGNETIZATION; POLARIMETERS; SYNCHROTRON RADIATION; TELESCOPES;

MAGNETIC FIELDS-POLARIZATION-TECHNIQUES; MAGNETIC-FIELDS-ISM; POLARIMETRIC-ISM; STRUCTURE-RADIO CONTINUUM:ISM; SYNCHROTRON EMISSIONS;

ASTROPHYSICS;

EID: 8644272515     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:200400042     Document Type: Article

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