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Interstellar Wind-Blown Bubbles
Published online by Cambridge University Press: 12 April 2016
Summary
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‘Classical’ stellar wind-driven bubbles are either energy or momentum driven, and evolve in smooth media containing only radial density gradients. Real bubbles are produced from winds from moving stars and which blow into non-homogeneous media. The resulting mixing of clump material can produce a variety of thermal, dynamical and chemical effects. In this review we discuss some of the modifications to classical bubbles which ensue, using observational examples where appropriate.
- Type
- II. Mechanical Energy Sources
- Information
- International Astronomical Union Colloquium , Volume 120: Structure and Dynamics of the Interstellar Medium , 1989 , pp. 136 - 145
- Copyright
- Copyright © Springer-Verlag 1989
References
Barlow, M. J., Smith, L. J. and Willis, A. J., 1981. Mon. Not. R. astr. Soc, 196, 101.Google Scholar
Charnley, S. B., Dyson, J. E., Hartquist, T. W. and Williams, D. A., 1988a. Mon. Not. R. astr. Soc, 231, 269.CrossRefGoogle Scholar
Charnley, S. B., Dyson, J. E., Hartquist, T. W. and Williams, D. A., 1988b. Mon. Not. R. astr. Soc, 235, 1257.Google Scholar
Charnley, S. B., Dyson, J. E., Hartquist, T. W. and Williams, D. A., 1989. Mon. Not. R. astr. Soc. (in press).Google Scholar
Dyson, J. E., 1981. In Investigating the Universe, ed. Kahn, F. D., p.125. D. Reidel Publ. Co., Dordrecht, Holland.Google Scholar
Dyson, J. E. and Smith, L.J., 1986. In Cosmical Gas Dynamics, ed. Kahn, F. D., p.173. VNU Science Press, Utrecht, Holland.Google Scholar
Genzel, R., Downes, D., Schneps, M. H., Reid, M. J., Moran, J. M., Kogan, L. R., Kostenko, V. L., Matveyenko, L. I. and Ronnaug, B., 1981. Astrophys. J., 247, 1039.Google Scholar
Hartquist, T. W., Dyson, J. E., Pettini, M. and Smith, L. J., 1986. Mon. Not. R. astr. Soc, 221, 715.Google Scholar
Innes, D. E., Giddings, J. R. and Falle, S. A. E. G., 1986. In Cosmical Gas Dynamics, ed. Kahn, F. D., p.143. VNU Science Press, Utrecht, Holland.Google Scholar
Maeder, A., 1984. In Observational Tests of the Stellar Evolution Theory, IAU Symposium 105, eds. Maeder, A. and Renzini, A., p.299. D. Reidel Publ. Co., Dordrecht, Holland.Google Scholar
Meaburn, J., Hartquist, T. W. and Dyson, J. E., 1988. Mon. Not. R. astr. Soc, 230, 243.CrossRefGoogle Scholar
Smith, L. J., Pettini, M., Dyson, J. E. and Hartquist, T. W., 1984. Mon. Not. R. astr. Soc, 211, 679.Google Scholar
Smith, L. J., Pettini, M., Dyson, J. E. and Hartquist, T. W., 1988. Mon. Not. R. astr. Soc, 234, 625.Google Scholar
Weaver, R., McCray, R., Castor, J., Shapiro, P. and Moore, R., 1977. Astrophys. J., 218, 377.Google Scholar
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