Time dependent outflows from accreting magnetic YSOs

Details Time dependent outflows from accreting magnetic YSOs Time dependent outflows from accreting magnetic YSOs

Apr 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998aipc..431..533g&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, Accretion And Accretion Disks, Magnetohydrodynamics And Plasmas

Scientific paper

We present high resolution numerical magnetohydrodynamic (MHD) simulation results of the interaction between a magnetic young stellar object (YSO) and a surrounding conducting accretion disk. A two component outflow arises, consisting of a high velocity, collimated jet and a slower, poorly collimated disk wind. The stellar magnetosphere undergoes forced oscillations in radius, with each oscillation correlating with the formation of an optical knot in the jet and with major magnetic reconnection and accretion events.

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