A new YSO outflow model, jet simulations, and their emission

Thibaut Lery*

*Corresponding author for this work

    Research output: Contribution to journalConference articlepeer-review

    Abstract

    In the usual theoretical picture of star formation a jet is ejected from a magnetized accretion disk, with a molecular outflow being driven either by the jet or by a wider wind coming from the disk. We propose an alternative unified model for the flows surrounding YSOs. In addition to a central accretion-ejection engine driving the jet, the molecular outflow is powered by the infalling matter and follows a circulation pattern around the central object without being entrained by an outflow. 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.

    Original languageEnglish (US)
    Pages (from-to)66-70
    Number of pages5
    JournalRevista Mexicana de Astronomia y Astrofisica: Serie de Conferencias
    Volume13
    StatePublished - Dec 1 2002
    EventEmission Lines from Jet Flows - Isla Mujeres, Mexico
    Duration: Nov 13 2000Nov 17 2000

    Keywords

    • ISM: jets and outflows
    • Magnetohydrodynamics
    • Stars: pre-main-sequence

    ASJC Scopus subject areas

    • Space and Planetary Science
    • Astronomy and Astrophysics

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