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- W2010159552 abstract "We present 2. 4 resolution, high sensitivity radio continuum observations of the nearby spiral galaxy NGC 4258 in total intensity and linear polarization obtained with the Very Large Array at λ3.6 cm (8.44 GHz). The radio emission along the northern jet and the center of the galaxy is polarized and allows investigation of the mag- netic field. Assuming energy-equipartition between the magnetic field and the relativistic particles and distinguishing be- tween (1) a relativistic electron-proton jet and (2) a relativistic electron-positron jet, we obtain average magnetic field strengths of about (1) 310 µ Ga nd (2) 90µG. The rotation measure is determined to range from −400 to −800 rad/m 2 in the northern jet. Correcting the observed E-vectors of polarized intensity for Faraday rotation, the magnetic field along the jet turns out to be orientated mainly along the jet axis. An observed tilt with respect to the jet axis may indicate also a toroidal magnetic field component or a slightly helical magnetic field around the northern jet." @default.
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- W2010159552 date "2004-06-01" @default.
- W2010159552 modified "2023-09-27" @default.
- W2010159552 title "The magnetic field along the jets of NGC 4258. as deduced from high frequency radio observations" @default.
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