Cool Stars 14 - Submitted Abstract # 85 This version created on 05 October 2006 Proposed New Members of the HD 141569 Association Alicia Aarnio, Vanderbilt University Alycia Weinberger, Carnegie Institution of Washington Keivan Stassun, Vanderbilt University We present results of a search for a young stellar moving group associated with the star HD141569A, the B9.5Ve primary member of a triple star system at 100pc. The age of this system is 5+/-3Myr as determined from placing the M-type companions on pre-main sequence evolutionary tracks. We have searched a 30 degree region around HD141569 for ROSAT sources with Tycho-2 proper motions consistent with that of HD141569. This search yielded 48 stars, some of which are known T-Tauri stars. Using visual wavelength echelle spectra from the Las Campanas and Lick Observatories, we found five stars with Li I equivalent widths indicative of youth as well as a greater than 50% probability of 3-dimensional galactic (UVW) comovement. We also discuss the sample in the context of nearby subgroups in the Scorpius-Centaurus complex. ----------------------------------