Abstract
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.
| Original language | English |
|---|---|
| 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 |
| Pages | 551-553 |
| Number of pages | 3 |
| ISBN (Print) | 9783642005756 |
| DOIs | |
| Publication status | Published - 2009 |
| Externally published | Yes |