articleAnnual Review of Astronomy and AstrophysicsAug 17, 2004GREEN OA

Interstellar Turbulence I: Observations and Processes

BGBruce G. ElmegreenJSJohn Scalo

IBM (United States) · The University of Texas at Austin

Indexed inarxivcrossref

Abstract

▪ Abstract Turbulence affects the structure and motions of nearly all temperature and density regimes in the interstellar gas. This two-part review summarizes the observations, theory, and simulations of interstellar turbulence and their implications for many fields of astrophysics. The first part begins with diagnostics for turbulence that have been applied to the cool interstellar medium and highlights their main results. The energy sources for interstellar turbulence are then summarized along with numerical estimates for their power input. Supernovae and superbubbles dominate the total power, but many other sources spanning a large range of scales, from swing-amplified gravitational instabilities to cosmic…

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Authors

2
  • BG
    Bruce G. ElmegreenCorresponding

    IBM (United States)

  • JS
    John Scalo

    The University of Texas at Austin

Topics & keywords

Keywords
  • Turbulence
  • Interstellar medium
  • Magnetohydrodynamic turbulence
  • Magnetohydrodynamics
  • K-epsilon turbulence model
  • K-omega turbulence model
  • Interstellar cloud
  • Turbulence kinetic energy
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