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- W39694998 abstract "By VLBI astrometry, we show that the two RSCVn type binaries, UX Ari and σ 2 CrB, have a preferred site of radio emission which is the intra-system region. It is known that radio emission from these stars is from the gyro-synchrotron process associated with large-scale magnetic fields. High gravity in the intra-system region might favor dense magnetic loops. Interactions in this region between loops attached to the surfaces of the two stellar components might produce reconnections required for electron acceleration." @default.
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- W39694998 date "1996-01-01" @default.
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- W39694998 title "VLBI for probing large-scale magnetic structures of stars" @default.
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- W39694998 doi "https://doi.org/10.1017/s0074180900083200" @default.
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