Cool Stars 14 - Submitted Abstract # 125 This version created on 05 October 2006 Doppler Imaging of T Tauri Stars in the TW Hya Association Mairead Skelly, Imperial College London Yvonne Unruh, Imperial College London Andrew Collier Cameron, University of St. Andrews John Barnes, University of Hertfodrshire Jean-Francois Donati, Observatoire Midi-Pyrenees, Toulouse Warwick Lawson, UNSW@ADFA, Canberra Brad Carter, University of Southern Queensland We present Doppler images of two rapidly rotating diskless T Tauri stars from the TW Hydrae association - TWA 6 and TWA 17. These images have been constructed using spectra from AAT/UCLES. The total observing time was 3+3 nights, with a 5 night gap. As three nights allows full phase coverage of both stars, two maps of each can be produced. Least Squares Deconvolution was applied to make use of a large number of spectral lines to achieve the high signal to noise ratios required for Doppler imaging. Using the deconvolved lines, we measure a projected equatorial rotation velocity of 75 km/s for TWA 6, which is somewhat greater than the previously reported value of 55 km/s. The deconvolved lines enable reconstruction of surface spot distributions of the stellar surfaces. We present here surface maps of the two stars and a discussion of the stellar parameters. ----------------------------------