Tracing magnetic field with synchrotron polarization gradients: parameter study
نویسندگان
چکیده
منابع مشابه
Magnetic Field Structure from Synchrotron Polarization
Total magnetic fields in spiral galaxies, as observed through their total synchrotron emission, are strongest (up to ≃ 30 μG) in the spiral arms. The degree of radio polarization is low; the field in the arms must be mostly turbulent or tangled. Polarized synchrotron emission shows that the resolved regular fields are generally strongest in the interarm regions (up to ≃ 15 μG), sometimes formin...
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ژورنال
عنوان ژورنال: Monthly Notices of the Royal Astronomical Society
سال: 2019
ISSN: 0035-8711,1365-2966
DOI: 10.1093/mnras/stz1176