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Line Profile microvariability and wind structure for OB stars
Published online by Cambridge University Press: 12 July 2011
Abstract
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We report the results of a search for line profile variability (LPV) in the spectra of OB stars. The wavelets were used for looking for the irregular LPV in spectra of program stars. We connect the appearance of irregular details in the LPV with the formation and dissipation of the small-scale substructures (clumps) in the wind.
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- Copyright © International Astronomical Union 2011
References
Kholtygin, A. F., Monin, D. N., Surkov, A. E., & Fabrika, S. N. 2003, Astron. Lett., 29, 175CrossRefGoogle Scholar
Kholtygin, A. F., Burlakova, T. E., Fabrika, S. N., Valyavin, G. G. et al. 2006, Astron. Rep., 50, 887CrossRefGoogle Scholar
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