POSTER PAPER 3.06

Time Series Spectropolarimetry of T Tauri Stars
Jeff A. Valenti, Christopher M. Johns--Krull, Artie P. Hatzes

Institute: Space Telescope Science Institute
Institute: Rice University
Institute: Thuringer Landessternwarte Tautenburg
Contact Email: valenti@stsci.edu

Abstract: We present 6 nights of spectropolarimetry and simultaneous photometry for the T Tauri stars AA Tau, BP Tau, DF Tau, and DK Tau. We determine net longitudinal magnetic field globally using photospheric absorption lines and in accretion zones using the 5876 A He I line. We compare changes in magnetic field, broad band photometry, absorption line depths (veiling), line profile morphology, emission line strength, velocity shifts, and line asymmetry. The data constrain magnetic and accretion geometry.

Time Series Spectropolarimetry of T Tauri Stars [PDF - Type 1 fonts]

Time Series Spectropolarimetry of T Tauri Stars [PS]


Index Keywords: AA Tau; BP Tau; DF Tau; DK Tau; T Tauri Stars; Accretion; Polarimetry; Veiling

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Manuscript submitted: 2001-Oct-30
"The Future of Cool-Star Astrophysics", 2003, Eds. A. Brown, G. M. Harper, & T. R. Ayres. Proceedings of 12th Cambridge Workshop on Cool Stars, Stellar Systems, & The Sun,
© 2003 University of Colorado.