We report the results of searching for the line profile variability (lpv) in the spectra of OB stars. The wavelets were used for looking for the irregular lpv in the spectra of program stars. We connect the appearance of irregular details in the lpv with the formation and destruction the small-scale substructures (clumps) in the wind.
Язык оригиналаанглийский
Страницы (с-по)200-201
ЖурналPROCEEDINGS OF SYMPOSIA OF THE INTERNATIONAL ASTRONOMICAL UNION
Том6
Номер выпускаSymp. S272
DOI
СостояниеОпубликовано - 2010

ID: 5218699