We present our latest three-dimensional time-dependent simulations of T Tauri jets launched from the surface of Keplerian disks, in an effort to extend the calculations to scales probed by HST (~50 AU) thereby allowing a direct comparison between simulations and observations. We explore the long-term stability the simulated jets were able to achieve. We plan to produce toroidal velocity maps that can be directly compared with the observed radial velocity shifts in several T Tauri jets that are suggestive of jet rotation.
|Title of host publication||Protostellar jets in context|
|Editors||K. Tsinganos, T. Ray, M. Stute|
|Place of Publication||Heidelberg ; New York|
|Publisher||Springer, Springer Nature|
|Number of pages||3|
|Publication status||Published - 2009|