PMS 3D work

Well suited to 3D - compact emission knots in extended emission regions (HH objects); high radial velocities, range of ionization conditions (shock diagnostics)
Work on DG Tau jet with Oasis (Lavalley, Dougados, Cabrit)
High extinction in circumstellar regions of Class II-III protosars. Near-IR spectrometry well suited - shocked molecular H lines at 2.1micron
Ideal application of AO + 3D for tracing jets close to bright stars - homing in on the origin of jets, small scale structure of shock regions

Well suited to 3D - compact emission knots in extended emission regions (HH objects); high radial velocities, range of ionization conditions (shock diagnostics)