The nature of turbulence in OMC1 at the scale of star formation: observations and simulations

by M. Gustafsson, A. Brandenburg, J. L. Lemaire, & D. Field

  • The structure functions of OMC1 are computed.
  • Using extended self-similarity, power laws are recovered at scales down to 160AU.
  • Deviations from supersonic turbulence simulations are due to preferentially observing the shocked gas.

    Reference:

  • Gustafsson, M., Brandenburg, A., Lemaire, J. L., & Field, D.: 2006, ``The nature of turbulence in OMC1 at the star forming scale: observations and simulations,'' Astron. Astrophys. 454, 815-825 (astro-ph/0512214, ADS, HTML, PDF)
  • Brandenburg, A., Korpi, M. J., & Mee, A. J.: 2007, ``Thermal instability in shearing and periodic turbulence,'' Astrophys. J. 654, 945-954 (astro-ph/0604244, ADS, DOI, HTML, PDF)


    Run directories:

  • Figs. 3-5: Run 1,
  • Figs. 6+7: Run 3,
  • Fig. 8: Run 2.


    Axel Brandenburg
    $Date: 2017/07/11 09:26:04 $, $Author: brandenb $, $Revision: 1.4 $