Time variable funnel flows

Details Time variable funnel flows Time variable funnel flows

May 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007iaus..243...71a&link_type=abstract

Star-Disk Interaction in Young Stars, Proceedings of the International Astronomical Union, IAU Symposium, Volume 243, p. 71-82

Astronomy and Astrophysics

Astronomy

3

Stars: Pre–Main-Sequence, Stars: Magnetic Fields, Circumstellar Matter, Accretion

Scientific paper

Magnetospheric accretion models are the current consensus to explain the main observed characteristics of classical T Tauri stars. In recent years the concept of a static magnetosphere has been challenged by synoptic studies of classical T Tauri stars that show strong evidence for the accretion process to be dynamic on several timescales and governed by changes in the magnetic field configuration. At the same time numerical simulation results predict evolving funnel flows due to the interaction between the stellar magnetosphere and the inner disk region. In this contribution we will focus on the main recent observational evidences for time variable funnel flows and compare them with model predictions.

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