Interstellar Turbulence I: Observations and Processes
IBM (United States) · The University of Texas at Austin
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…
Citation impact
- FWCI
- 29.06
- Percentile
- 100%
- References
- 401
Authors
2- BGBruce G. ElmegreenCorresponding
IBM (United States)
- JSJohn Scalo
The University of Texas at Austin
Topics & keywords
- Turbulence
- Interstellar medium
- Magnetohydrodynamic turbulence
- Magnetohydrodynamics
- K-epsilon turbulence model
- K-omega turbulence model
- Interstellar cloud
- Turbulence kinetic energy