Differential rotation and magnetic fields of T Tauri stars

Details Differential rotation and magnetic fields of T Tauri stars Differential rotation and magnetic fields of T Tauri stars

Apr 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998aipc..431..509k&link_type=abstract

Accretion processes in astrophysical systems: Some like it hot! - eigth astrophysics conference. AIP Conference Proceedings, Vo

Astronomy and Astrophysics

Astrophysics

Pre-Main Sequence Objects, Young Stellar Objects And Protostars, Stellar Characteristics And Properties, Magnetohydrodynamics And Plasmas

Scientific paper

Results of recent investigations indicate that T Tauri stars rotate rigidly [1]. Due to this lack of differential rotation, the stellar magnetic field can not be maintained by a solar-type αΩ dynamo. We have therefore worked out a model of an α2 dynamo and solved the induction equation in three dimensions. The resulting magnetic field is non-axisymmetric and does not show any activity cycle.

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