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Differential line-shifts

  • William Buscombe
2. Observed Properties of Stellar Turbulence
Part of the Lecture Notes in Physics book series (LNP, volume 114)

Keywords

Velocity Displacement Excitation Potential Bolometric Luminosity Luminosity Class Photospheric Line 
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. Aydin, C. 1972, Astron. Astrophys. 19, 369.Google Scholar
  2. Conti, P. 1977, Astrophy. J. 215, 561.CrossRefGoogle Scholar
  3. Hutchings, J.B. 1968, Mon. Not. R. Astron. Soc. 141, 219.Google Scholar
  4. Imhoff, C.L. 1976, thesis, Ohio State University.Google Scholar
  5. Merrill, P.W. 1960, in Stellar Atmospheres (ed. J.L. Greenstein), U. of Chicago Press, p. 516.Google Scholar
  6. Morton, D.C. 1976, Astrophys. J. 203, 386.CrossRefGoogle Scholar
  7. Rosendhal, J.D. 1973, Astrophys. J. 186, 909.CrossRefGoogle Scholar
  8. Sargent, W.L.W. and P.S. Osmer 1969, in Mass Loss from Stars (ed. M. Hack), Dordrecht: Reidel, p. 57.Google Scholar
  9. Smolinski, J.; J.L. Climenhaga, H. Funakawa, and J.M. Fletcher, 1979 Internat. Astronom. Un. Circular no. 3382.Google Scholar

Copyright information

© Springer-Verlag 1980

Authors and Affiliations

  • William Buscombe
    • 1
  1. 1.Northwestern UniversityEvanstonUSA

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