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.
Similar content being viewed by others
References
A. F. J. Moffat, S. Lépine, R. N. Henriksen, and C. Robert, Astrophys. Space Sci. 216, 55 (1994).
T. Eversberg, S. Lépine, and A. F. J. Moffat, Astrophys. J. 494, 799 (1998).
A. M. Cherepashchuk, Astron. Zh. 67, 955 (1990) [Sov. Astron. 34, 481 (1990)].
S. Marchenko, A. F. J. Moffat, et al., in Wolf-Rayet Phenomena in Massive Stars at Galaxies (IAU Symposium 193), p. 47.
A. M. Cherepashchuk, J. A. Eaton, and Kh. F. Khaliullin, Astrophys. J. 281, 774 (1984).
I. I. Antokhin, A. F. Kholtygin, and A. M. Cherepashchuk, Astron. Zh. 65, 558 (1988) [Sov. Astron. 32, 285 (1988)].
S. Lépine, Astrophys. Space Sci. 221, 371 (1993).
S. Lépine, A. F. J. Moffat, and R. N. Henriksen, Astrophys. J. 466, 392 (1996).
S. Lépine and A. F. J. Moffat, Astrophys. J. 514, 909 (1999).
F. V. Kostenko and A. F. Kholtygin, Astrofizika 42, 373 (1999).
A. F. Kholtygin, ASP Conf. Ser. 204, 231 (2000).
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.
V. V. Sobolev, A Course in Theoretical Astrophysics [in Russian] (Nauka, Moscow, 1975), p. 354.
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.
Kh. F. Khaliullin and A. M. Cherepashchuk, Itogi Nauki Tekh., Ser. Astron. 21, 5 (1982).
J. I. Castor and H. J. G. L. M. Lamers, Astrophys. J., Suppl. Ser. 39, 481 (1979).
A. F. J. Moffat, L. Drissen, R. Lamontagne, and C. Robert, Astrophys. J. 334, 1038 (1988).
N. M. Astaf’eva, Usp. Fiz. Nauk 166(11), 145 (1996) [Phys. Usp. 39, 1085 (1996)].
Author information
Authors and Affiliations
Additional information
__________
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.
Rights and permissions
About this article
Cite this article
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
Received:
Issue Date:
DOI: https://doi.org/10.1134/1.1361320