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Modeling of rapid variability in the spectral line profiles of Wolf-Rayet stars

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Abstract

Profiles of variable emission lines in the spectra of Wolf-Rayet stars are calculated using a stochastic cloud model for the inhomogeneous atmospheres of early-type stars. The model assumes that most of the line flux is formed in cold, dense condensations (clouds) that move through a rarified inter-cloud medium whose density monotonically decreases outwards. The formation of clouds is taken to be stochastic. Wavelet analysis is used to estimate the parameters of cloud ensembles. The model can reproduce the general pattern of line-profile variability observed in the spectra of Wolf-Rayet stars.

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References

  1. A. F. J. Moffat, S. Lépine, R. N. Henriksen, and C. Robert, Astrophys. Space Sci. 216, 55 (1994).

    Article  ADS  Google Scholar 

  2. T. Eversberg, S. Lépine, and A. F. J. Moffat, Astrophys. J. 494, 799 (1998).

    Article  ADS  Google Scholar 

  3. A. M. Cherepashchuk, Astron. Zh. 67, 955 (1990) [Sov. Astron. 34, 481 (1990)].

    ADS  Google Scholar 

  4. S. Marchenko, A. F. J. Moffat, et al., in Wolf-Rayet Phenomena in Massive Stars at Galaxies (IAU Symposium 193), p. 47.

  5. A. M. Cherepashchuk, J. A. Eaton, and Kh. F. Khaliullin, Astrophys. J. 281, 774 (1984).

    Article  ADS  Google Scholar 

  6. I. I. Antokhin, A. F. Kholtygin, and A. M. Cherepashchuk, Astron. Zh. 65, 558 (1988) [Sov. Astron. 32, 285 (1988)].

    ADS  Google Scholar 

  7. S. Lépine, Astrophys. Space Sci. 221, 371 (1993).

    Google Scholar 

  8. S. Lépine, A. F. J. Moffat, and R. N. Henriksen, Astrophys. J. 466, 392 (1996).

    ADS  Google Scholar 

  9. S. Lépine and A. F. J. Moffat, Astrophys. J. 514, 909 (1999).

    ADS  Google Scholar 

  10. F. V. Kostenko and A. F. Kholtygin, Astrofizika 42, 373 (1999).

    Google Scholar 

  11. A. F. Kholtygin, ASP Conf. Ser. 204, 231 (2000).

    ADS  Google Scholar 

  12. D. J. Hillier, in Wolf-Rayet Stars: Binaries, Colliding Winds, Evolution (IAU Symposium 163), Ed. by K. A. van der Hucht and P. M. Williams (Kluwer, Dordrecht, 1995), p. 116.

    Google Scholar 

  13. V. V. Sobolev, A Course in Theoretical Astrophysics [in Russian] (Nauka, Moscow, 1975), p. 354.

    Google Scholar 

  14. A. F. Kholtygin, in Wolf-Rayet Stars: Binaries, Colliding Winds, Evolution (IAU Symposium 163), Ed. by K. A. van der Hucht and P. M. Williams (Kluwer, Dordrecht, 1995), p. 160.

    Google Scholar 

  15. Kh. F. Khaliullin and A. M. Cherepashchuk, Itogi Nauki Tekh., Ser. Astron. 21, 5 (1982).

    Google Scholar 

  16. J. I. Castor and H. J. G. L. M. Lamers, Astrophys. J., Suppl. Ser. 39, 481 (1979).

    Article  ADS  Google Scholar 

  17. A. F. J. Moffat, L. Drissen, R. Lamontagne, and C. Robert, Astrophys. J. 334, 1038 (1988).

    Article  ADS  Google Scholar 

  18. N. M. Astaf’eva, Usp. Fiz. Nauk 166(11), 145 (1996) [Phys. Usp. 39, 1085 (1996)].

    Google Scholar 

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Translated from Astronomicheski\(\overset{\lower0.5em\hbox{$\smash{\scriptscriptstyle\smile}$}}{l}\) Zhurnal, Vol. 78, No. 4, 2001, pp. 333–340.

Original Russian Text Copyright © 2001 by Kudryashova, Kholtygin.

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Kudryashova, N.A., Kholtygin, A.F. Modeling of rapid variability in the spectral line profiles of Wolf-Rayet stars. Astron. Rep. 45, 287–293 (2001). https://doi.org/10.1134/1.1361320

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  • DOI: https://doi.org/10.1134/1.1361320

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