Skip to main content

Magnetic Fields in Diffuse HI and Molecular Clouds

  • Chapter
  • First Online:
Cosmic Magnetic Fields

Part of the book series: Lecture Notes in Physics ((LNP,volume 664))

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.

This is a preview of subscription content, log in via an institution to check access.

Access this chapter

Institutional subscriptions

Preview

Unable to display preview. Download preview PDF.

Unable to display preview. Download preview PDF.

References

Download references

Author information

Authors and Affiliations

Authors

Editor information

Richard Wielebinski Rainer Beck

Rights and permissions

Reprints and permissions

About this chapter

Cite this chapter

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

Download citation

  • DOI: https://doi.org/10.1007/3540313966_7

  • Published:

  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-540-24175-1

  • Online ISBN: 978-3-540-31396-0

  • eBook Packages: Physics and AstronomyPhysics and Astronomy (R0)

Publish with us

Policies and ethics