Circumstellar discs around Herbig Ae/Be and Vega-type stars and local magnetic fields

Details Circumstellar discs around Herbig Ae/Be and Vega-type stars and local magnetic fields Circumstellar discs around Herbig Ae/Be and Vega-type stars and local magnetic fields

Nov 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aspc..337..342y&link_type=abstract

The Nature and Evolution of Disks Around Hot Stars, ASP Conference Series, Vol. 337, Proceedings of a meeting held 7-9 July 2004

Computer Science

Scientific paper

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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