The Environment of YSO Jets

Thibaut Lery, Céline Combet, Gareth Murphy

Research output: Contribution to journalJournal articleResearchpeer-review

Abstract

It is commonly accepted that stars form in molecular clouds by the gravitational collapse of dense gas. However, it is precisely not the infalling but the outflowing material that is primarily observed. Outflow motions prevail around both low and high mass young stellar objects. We present here results from a family of self-similar models that could possibly help to understand this paradox. The models take into account the heating of the central protostar for the deflection and acceleration of the gas. The models make room for all the ingredients observed around the central objects, i.e. molecular outflows, fast jets, accretion disks and infalling envelopes. We suggest that radiative heating and magnetic field may ultimately be the main energy sources driving outflows for both low and high mass stars. The models show that the ambient medium surrounding the jet is unhomogeneous in density, velocity, magnetic field. Consequently, we suggest that jets and outflows have a prehistory that is inprinted in their environment, and that this should have direct consequences on the setting of jet numerical simulations
Original languageEnglish
JournalAstrophysics and Space Science
Volume293
Issue number1-2
Pages (from-to)263-269
ISSN0004-640X
DOIs
Publication statusPublished - 2004
Externally publishedYes

Keywords

  • ISM
  • Jets
  • Outflows
  • Star formation

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