The effects of electron scattering and wind clumping for early emission line stars

摘要: Using two independent codes, a detailed study of the influence electron scattering on line profiles arising from stellar winds around early emission stars have been made. These calculations indicate that assumption isotropic gives acceptable answers when compared with more accurate using dipole phase function. On other hand use angle-averaged redistribution functions can noticeably affect strength predict wings. In addition it is shown velocity adopted for Doppler absorption profile dramatically wings optically thick throughout most its formation region