Generation of ``turbulence'' in molecular cloud by HH objects

Details Generation of ``turbulence'' in molecular cloud by HH objects Generation of ``turbulence'' in molecular cloud by HH objects

Sep 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aipc..784..730d&link_type=abstract

MAGNETIC FIELDS IN THE UNIVERSE: From Laboratory and Stars to Primordial Structures. AIP Conference Proceedings, Volume 784, pp

Physics

Interstellar Molecular Clouds, Magnetohydrodynamics, Turbulence, Pre-Main-Sequence Stars, Molecular Clouds, H2 Clouds, Dense Clouds, And Dark Clouds, Magnetohydrodynamics And Plasmas, Pre-Main Sequence Objects, Young Stellar Objects And Protostars

Scientific paper

Using simulations of high density clumps (which could be the result of a time-dependent ejection from a young, low mass star) propagating in a uniform medium, we studied (De Colle & Raga) the transfer of momentum and energy from a clump to the molecular cloud. We find that the presence of the magnetic field facilitates the transport of momentum and energy in the direction perpendicular to the jet motion, and in this way jets can generate turbulence in the surrounding, magnetized cloud.

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