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Paper: Circumstellar Discs Around Herbig Ae/Be and Vega-type Stars and Local Magnetic Fields
Volume: 337, The Nature and Evolution of Disks Around Hot Stars
Page: 342
Authors: Yudin, R.V.
Abstract: There is a reason to believe that during the evolution the compression of circumstellar (CS) envelopes around young stars takes place along the line-of force of local magnetic fields that results to the formation of CS discs. Nowadays, there is a consensus that most young stellar objects exhibit such CS dusty discs. To verify this hypothesis we investigate the behaviour of Herbig Ae/Be stars in the q,u-plane of Stokes parameters.
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