Abstract
The diffuse interstellar HI is the matrix within which many molecular clouds reside and the medium that soaks up the energy injected by sources such as supernovae and stellar winds. This energy stimulates turbulence in the HI, which cascades up the turbulent wavenumber spectrum. The spectral wavelengths extend all the way down to scales most easily quoted in Astronomical Units. HI and molecular clouds enjoy a synergistic relationship, with turbulent energy, angular momentum, magnetic fields, and matter flowing across the boundaries in both directions. The molecular clouds form stars, which in turn act as energy sources to round the circle and make star formation a feedback process.
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Heiles, C., Crutcher, R. Magnetic Fields in Diffuse HI and Molecular Clouds. In: Wielebinski, R., Beck, R. (eds) Cosmic Magnetic Fields. Lecture Notes in Physics, vol 664. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3540313966_7
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