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VLBI for probing large-scale magnetic structures of stars
Published online by Cambridge University Press: 25 May 2016
Abstract
By VLBI astrometry, we show that the two RSCVn type binaries, UX Ari and σ2 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.
- Type
- Session II: “Direct Mapping: The Last Frontier”
- Information
- Symposium - International Astronomical Union , Volume 176: Stellar Surface Structure , 1996 , pp. 173 - 180
- Copyright
- Copyright © Kluwer 1996