Line profile microvariability and wind structure for OB stars

dc.contributor.authorKholtygin, Alexander F.
dc.contributor.authorFabrika, Sergei N.
dc.contributor.authorSudnik, N. P.
dc.date.accessioned2016-12-11T12:31:21Z
dc.date.available2016-12-11T12:31:21Z
dc.date.issued2011
dc.description.abstractWe 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.ru_RU
dc.identifier.urihttp://elib.bspu.by/handle/doc/17606
dc.language.isoenru_RU
dc.relation.ispartofseriesProc. IAU Symposium;No. 272, p. 200
dc.subjectБГПУru_RU
dc.subjectstarsru_RU
dc.subjectearly-typeru_RU
dc.subjectother variablesru_RU
dc.subjectline profilesru_RU
dc.subjectwindsru_RU
dc.subjectoutflowsru_RU
dc.titleLine profile microvariability and wind structure for OB starsru_RU
dc.typeArticleru_RU

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