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On the virial theorem for turbulent molecular clouds

McKee, Christopher F., Zweibel, Ellen G.·1992·The Astrophysical Journal

Abstract

An Eulerian, rather than Lagrangian, form of the virial theorem is derived for a turbulent, magnetized cloud embedded in a steady, turbulent, low-density intercloud medium. The role of turbulent pressure in cloud confinement is clarified, and it is shown that, in the absence of a magnetic field, a cloud can be at a somewhat lower pressure than the intercloud medium. Simple forms for the magnetic term in the virial equation are obtained. Radiation pressure is considered; its effects are relatively small under average conditions in the interstellar medium. Under typical conditions, external pressure and magnetic fields are shown to have a relatively small effect on virial estimates of the mass of self-gravitating clouds.

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Metadata

Authors
McKee, C. F., & Zweibel, E. G.
Venue
The Astrophysical Journal
Published
1992-11
Volume
399
Pages
551
ISSN
  • 0004-637X (ISSN-L)
  • 1538-4357
OpenAlex
W1991741105
Cited by
158
References
0
FWCI
0.66
Type
journal article
Language
en
Open access
closed

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CoChat. (2026). Citation check: On the virial theorem for turbulent molecular clouds. https://app.cochat.ai/papers/10.1086/171946
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McKee, C. F., & Zweibel, E. G. (1992). On the virial theorem for turbulent molecular clouds. The Astrophysical Journal. https://doi.org/10.1086/171946

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Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.