Hostname: page-component-586b7cd67f-t7fkt Total loading time: 0 Render date: 2024-11-30T04:39:23.075Z Has data issue: false hasContentIssue false
  • English
  • Français

The fluctuation theory of the stellar mass loss

Published online by Cambridge University Press:  12 April 2016

C.D. Andriesse
C.D. Andriesse*
Affiliation:
Kapteyn Sterrenwacht, University of Groningen

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

That we cannot give a justification – or sufficient reasons – for our guesses does not mean that we may not have guessed the truth.

K.R. Popper

If studied in detail, the mass flows from the stars appear to be variable. “Mere inspection of solar wind data reveals large variations on a time scale of several days” (Hundhausen, 1972). Also, “it is obvious that mass loss from hot stars is not a stationary phenomenon but that variations on short timescale occur” (de Jager et. al., 1979). And a cool supergiant has “a photosphere fluctuating in both brightness and radial velocity, (and) an expanding chromosphere … uncoupled from motions in the photosphere” (Goldberg, 1979).

Type
Session IV - Winds From Late Type Stars: Theory
Information
International Astronomical Union Colloquium , Volume 59: Effects of Mass Loss on Stellar Evolution , 1981 , pp. 213 - 227
Copyright
Copyright © Reidel 1981

References

Andriesse, CD.: 1979, Astrophys. Space Sci. 61, 205.Google Scholar
Andriesse, CD.: 1980a, Astrophys. Space Sci. 67, 461.Google Scholar
Andriesse, CD.: 1980b, Astrophys. Space Sci. 72, 167.Google Scholar
Andriesse, CD.: 1980c, Mori. Not. R. astr. Soc. 192, 95.CrossRefGoogle Scholar
Baker, N.: 1972, in Stellar Evolution, H.-Y. Chiu and Muriel, A., Eds. (MIT Press, Cambridge, Mass.), pp. 163–164.Google Scholar
Becker, R.: 1961, Theorie der Wärme (Springer-Verlag, Berlin), pp. 266–267, 270.Google Scholar
Cannon, C.J., Thomas, R.N.: 1977, Astrophys. J. 211, 910.Google Scholar
Castor, J.I., Abbott, D.C, Klein, R.I.: 1975, Astrophys. J. 195, 157.CrossRefGoogle Scholar
de Jager, C, Lamers, H.J.G.L.M., Machetto, F., Snow, T.P.: 1979, Astron. Astrophys. 79, L28. Google Scholar
Fusi-Pecci, F., Renzini, A.: 1976, Astron. Astrophys. 46, 447.Google Scholar
Gilman, R.C: 1972, Astrophys. J. 178, 423.CrossRefGoogle Scholar
Goldberg, L.: 1979, Quart. J. R. astr. Soc. 20, 376.Google Scholar
Hearn, A.G.: 1975, Astron. Astrophys. 40, 355.Google Scholar
Hearn, A.G.: 1979, Astron. Astrophys. 79, LI.Google Scholar
Hundhausen, A.J.: 1972, Coronal Expansion and Solar Wind (Springer-Verlag, Berlin), p. 121.Google Scholar
Kiepenheuer, K.O.: 1968, in Mass Motion in Solar Flares and Related Phenomena, öhman, Y., Ed. (Wiley Interscience Div., New York), p. 125.Google Scholar
Landau, L.D., Lifshitz, E.M.: 1969, Statistical Physics (Pergamon Press,Oxford), p. 372.Google Scholar
Middleton, D.: 1960, Statistical Communication Theory (McGraw-Hill Book Comp., New York), pp. 438–466.Google Scholar
Pecker, J.C, Praderie, F., Thomas, R.N.: 1973, Astron. Astrophys. 29, 289.Google Scholar
Thomas, R.N.: 1973, Astron. Astrophys. 29, 297.Google Scholar
Thomas, R.N.: 1979, in Mass Loss and Evolution of 0-type Stars, Conti, P.S. and de Loore, C.W.H., Eds. (Reidei Pubi. Comp., Dordrecht), pp. 215–224.Google Scholar
Williams, I.P.: 1967, Mon. Not. R. astr. Soc. 136, 341.CrossRefGoogle Scholar