The position-velocity diagrams (PVDs) resulting from observations from DG-Tau stellar jet show features that might be originated by the jet rotation. Our synthetic PVDs obtained after post-processing numerical simulations of rotating jets performed by the PLUTO code, seem to confirm these features.
Numerical simulations of rotating jets: comparisons with observations / F. Rubini; L. Maurri; G. Inghirami; F. Bacciotti. - STAMPA. - 453:(In corso di stampa), pp. 391-392. (Intervento presentato al convegno Advances in computational astrophysics: methods and tools tenutosi a Cefalu, Italy nel June 13-17 2011).
Numerical simulations of rotating jets: comparisons with observations
RUBINI, FRANCESCO MARIO;
In corso di stampa
Abstract
The position-velocity diagrams (PVDs) resulting from observations from DG-Tau stellar jet show features that might be originated by the jet rotation. Our synthetic PVDs obtained after post-processing numerical simulations of rotating jets performed by the PLUTO code, seem to confirm these features.
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