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- W1520856948 abstract "In the usual theoretical picture of star formation a jet is ejected from a magnetized accretion disk, with a molecular outo w being driven either by the jet or by a wider wind coming from the disk. We propose an alternative unied model for the o ws surrounding YSOs. In addition to a central accretion-ejection engine driving the jet, the molecular outo w is powered by the infalling matter and follows a circulation pattern around the central object without being entrained by an outo w. Jets solutions from this model have been used as initial conditions for simulations of the propagation of pulsed jets. Synthetic maps from the jet simulations are presented." @default.
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- W1520856948 date "2002-06-01" @default.
- W1520856948 modified "2023-10-18" @default.
- W1520856948 title "A NEW YSO OUTFLOW MODEL, JET SIMULATIONS, AND THEIR EMISSION" @default.
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