The intrinsic magnetic field orientation in NGC 4631

Details The intrinsic magnetic field orientation in NGC 4631 The intrinsic magnetic field orientation in NGC 4631

Apr 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994a%26a...284..777g&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 284, no. 3, p. 777-792

Astronomy and Astrophysics

Astronomy

69

Galactic Radio Waves, Halos, Interstellar Magnetic Fields, Morphology, Polarized Radiation, Radio Astronomy, Radio Spectra, Spiral Galaxies, Astronomical Maps, Dependence, Faraday Effect, Fourier Transformation, Gas Flow, Gravitational Fields, Star Formation, Very Large Array (Vla), Wavelengths

Scientific paper

We present radio continuum measurements of the edge-on spiral galaxy NGC 4631 at 4.86 and 8.44 GHz. We discuss the morphology of the radio halo in total and polarized emission and its wavelength dependence. The rotation measure and intrinsic magnetic field orientation are determination using the two frequency pairs 4.86/8.44 GHz and 1.49/4.86 GHz, the latter with the help of published 1.49 GHz data. The results are summarized.

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