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Astrophysics and Space Science

, Volume 118, Issue 1–2, pp 383–393 | Cite as

The injection of energy into the interstellar medium by stars (invited review)

  • Christopher F. McKee
Section 4b: Galactic Structure

Abstract

Stars inject energy into the interstellar medium (ISM) by radiation, stellar winds, and supernova explosions. This energy injection causes the ISM to be inhomogeneous, which in turn alters the manner in which the energy is transferred through the ISM. A significant fraction of the energy is injected by massive stars, which formHii regions in the ISM. The structure and evolution ofHii regions in a cloudy medium deffers significantly from that in a homogeneous one. The strong stellar winds produced by massive stars form bubbles in the ISM, and the structure of these bubbles is often dominated by the structure of theHii region in which they are embedded. Finally, when the star explodes as a supernova, the evolution and appearance of the resulting remnant is determined by the structure of the bubble andHii region formed by the star during its lifetime.

Keywords

Radiation Significant Fraction Interstellar Medium Massive Star Stellar Wind 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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References

  1. Abbott, D. C.: 1982,Astrophys. J.,259, 282.Google Scholar
  2. Blair, W. P., Kirshner, R. P., and Chevalier, R. A.: 1981,Astrophys. J. 247, 879.Google Scholar
  3. Bruhweiler, F. C., Gull, T. R., Kafatos, M., and Sofia, S.: 1980,Astrophys. J. 238, L27.Google Scholar
  4. Castor, J., McCray, R., and Weaver, R.: 1975,Astrophys. J. 200, L107.Google Scholar
  5. Charles, P., Kahn, S., and McKee, C. F.: 1985.Astrophys. J. 295, 456.Google Scholar
  6. Chu, Y. H.: 1981,Astrophys. J. 249, 195.Google Scholar
  7. Clarke, J. N.: 1976,Monthly Notices Roy. Astron. Soc. 174, 393.Google Scholar
  8. Cowie, L. L., McKee, C. F., and Ostriker, J. P.: 1981,Astrophys. J. 247, 908.Google Scholar
  9. Cox, D. P. and Smith, B. W.: 1974,Astrophys. J. 189, L105.Google Scholar
  10. de Jong, T.: 1980, in P. A. Wayman (ed.),Highlights of Astronomy, D. Reidel Publ. Co., Dordrecht, Holland, Vol. 5, p. 301.Google Scholar
  11. Dopita, M. A.: 1979,Astrophys. J. Suppl. 40, 455.Google Scholar
  12. Elmegreen, B. G.: 1976,Astrophys. J. 205, 405.Google Scholar
  13. Field, G. B., Goldsmith, D. W., and Habing, H. J.: 1969,Astrophys. J. 155, L149.Google Scholar
  14. Hughes, J. P., Helfand, D. J., and Kahn, S. M.: 1984,Astrophys. J. 281, L25.Google Scholar
  15. Icke, V.: 1979,Astron. Astrophys. 78, 352.Google Scholar
  16. Lozinskaya, T. A.: 1982,Astrophys. Space Sci. 87, 313.Google Scholar
  17. Mathewson, D. S., Ford, V. L., Dopita, M. A., Tuohy, I. R., Long, K. S., and Helfand, D. J.: 1983, in I. J. Danziger and P. Gorenstein (eds.), ‘Supernova Remnants and Their X-Ray Emission’IAU Symp. 101, 541.Google Scholar
  18. McCray, R. and Snow, T. P.: 1979,Ann. Rev. Astron. Astrophys. 17, 213.Google Scholar
  19. McKee, C. F.: 1983, in I. J. Danziger and P. Gorenstein (eds.), ‘Supernova Remnants and Their X-Ray Emission’,IAU Symp. 101, 87.Google Scholar
  20. McKee, C. F. and Ostriker, J. P.: 1977,Astrophys. J. 218, 148.Google Scholar
  21. McKee, C. F., Van Buren, D., and Lazareff, B.: 1984,Astrophys. J. 278, L115.Google Scholar
  22. Mills, B. Y., Turtle, A. J., Little, A. G., and Durdin, J. M.: 1984,Australian J. Phys. 37, 321.Google Scholar
  23. Oort, J. H. and Spitzer, L.: 1955,Astrophys. J. 121, 6.Google Scholar
  24. Panagia, N.: 1973,Astron. J. 78, 929.Google Scholar
  25. Sedov, L.: 1969,Similarity and Dimensional Methods in Mechanics, Academic Press, New York.Google Scholar
  26. Seward, F. D. and Harnden, F. R.: 1982,Astrophys. J. 256, L45.Google Scholar
  27. Shull, P., Dyson, J. E., Kahn, F. D., and West, K.: 1985,Monthly Notices Roy. Astron. Soc. 212, 199.Google Scholar
  28. Spitzer, L.: 1978,Physical Processes in the Interstellar Medium, Wiley, New York.Google Scholar
  29. Tammann, G.: 1982, in M. J. Rees and R. Stoneham (eds.),Supernovae: A Survey of Current Research, D. Reidel Publ. Co., Dordrecht, Holland, p. 371.Google Scholar
  30. Tenorio-Tagle, G.: 1979,Astron. Astrophys. 71, 59.Google Scholar
  31. Van Buren, D., Lazareff, B., and McKee, C. F.: 1985 (in preparation).Google Scholar
  32. van den Bergh, S. and Kamper, K.: 1984,Astrophys. J. 280, L51.Google Scholar
  33. Weaver, R., McCray, R., Castor, J., Shapiro, P., and Moore, R.: 1977,Astrophys. J. 218, 377.Google Scholar
  34. Weiler, K. W.: 1983, in I. J. Danziger and P. Gorenstein (eds.),Supernova Remnants and Their X-Ray Emission, IAU Symp. 101, 299.Google Scholar

Copyright information

© D. Reidel Publishing Company 1986

Authors and Affiliations

  • Christopher F. McKee
    • 1
  1. 1.Departments of Physics and of AstronomyUniversity of CaliforniaBerkeleyU.S.A.

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