Skip to main content

Thank you for visiting nature.com. You are using a browser version with limited support for CSS. To obtain the best experience, we recommend you use a more up to date browser (or turn off compatibility mode in Internet Explorer). In the meantime, to ensure continued support, we are displaying the site without styles and JavaScript.

  • Letter
  • Published:

Self-gravity as an explanation of the fractal structure of the interstellar medium

Abstract

THE gas clouds of the interstellar medium have a fractal structure, the origin of which has generally been thought to lie in turbulence1,2. The energy of turbulence could come from galactic rotation at large scale, then cascade down to be dissipated on small scales by viscosity5,14; it has been suggested that such turbulence helps to prevent massive molecular clouds from collapsing in response to their own gravity15,16. Here we show that, on the contrary, self-gravity itself may be the dominant factor in making clouds fractal. We develop a field-theory approach to the structure of clouds, assuming them to be isothermal, and with only gravitational interactions; we find that the observed fractal dimension of the clouds arises naturally from this approach. Although this result does not imply that turbulence is not important, it does demonstrate that the fractal structure can be understood without it.

This is a preview of subscription content, access via your institution

Access options

Buy this article

Prices may be subject to local taxes which are calculated during checkout

Similar content being viewed by others

References

  1. Larson, R. B. Mon. Not. R. Astron. Soc. 194, 809–826 (1981).

    Article  ADS  CAS  Google Scholar 

  2. Falgarone, E., Phillips, T. G. & Walker, C. K. Astrophys. J. 378, 186–201 (1991).

    Article  ADS  CAS  Google Scholar 

  3. Scalo, J. M. in Instellar Processes (eds Hollenbach, D. J. & Thronson, H. A.) 349–392 (Reidel, Dordrecht, 1987).

    Book  Google Scholar 

  4. Wilson, K. G. Rev. Mod. Phys. 55, 583–600 (1983).

    Article  ADS  Google Scholar 

  5. Albeverio, S. & Høegh-Krohn, R. Commun. Math. Phys. 30, 171–200 (1973).

    Article  ADS  Google Scholar 

  6. Hubbard, J. Phys. Rev. Lett. 3, 77–78 (1959).

    Article  ADS  Google Scholar 

  7. Horwitz, G. & Katz, J. Astrophys. J. 222, 941–958 (1978).

    Article  ADS  Google Scholar 

  8. Pfenniger, D. & Combes, F. Astron. Astrophys. 285, 94–118 (1994).

    ADS  CAS  Google Scholar 

  9. Domb, C. & Green, M. S. Phase transitions and Critical Phenomena Vol. 6 (Academic, New York, 1976).

    Google Scholar 

  10. Morris, T. R. Phys. Lett. B 334, 355–362 (1994).

    Article  ADS  Google Scholar 

  11. Landau, L. D. & Lifshitz, E. M. Physique Statistique 4th edn (Mir-Ellipses, Paris, 1996).

    Google Scholar 

  12. Kleiner, S. C. & Dickman, R. L. Astrophys. J. 312, 837–847 (1987).

    Article  ADS  CAS  Google Scholar 

  13. Pfenniger, D., Combes, F. & Martinet, L. Astron. Astrophys. 285, 79–93 (1994).

    ADS  Google Scholar 

  14. Fleck, R. C. Astrophys. J. 458, 739–741 (1996).

    Article  ADS  Google Scholar 

  15. Henriksen, R. N. & Turner, B. E. Astrophys. J. 287, 200–207 (1984).

    Article  ADS  CAS  Google Scholar 

  16. Chièze, J.-P. Astron. Astrophys. 171, 225–232 (1987).

    ADS  Google Scholar 

Download references

Author information

Authors and Affiliations

Authors

Rights and permissions

Reprints and permissions

About this article

Cite this article

de Vega, H., Sánchez, N. & Combes, F. Self-gravity as an explanation of the fractal structure of the interstellar medium. Nature 383, 56–58 (1996). https://doi.org/10.1038/383056a0

Download citation

  • Received:

  • Accepted:

  • Issue Date:

  • DOI: https://doi.org/10.1038/383056a0

Comments

By submitting a comment you agree to abide by our Terms and Community Guidelines. If you find something abusive or that does not comply with our terms or guidelines please flag it as inappropriate.

Search

Quick links

Nature Briefing

Sign up for the Nature Briefing newsletter — what matters in science, free to your inbox daily.

Get the most important science stories of the day, free in your inbox. Sign up for Nature Briefing