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PHYSICAL PARAMETERS OF INHOMOGENEITIES IN WOLF-RAYET WINDS.
147 - 153.
Time-resolved spectroscopy has revealed small, systematically varying features superimposed on the broad emission lines of WR stars. We believe that these structures are due to inhomogeneities of emitting wind material propagating with the general wind. Here we suggest a common, but still unknown, origin for the intrinsic variations observed in WR stars.
|Title:||PHYSICAL PARAMETERS OF INHOMOGENEITIES IN WOLF-RAYET WINDS|
|UCL classification:||UCL > School of BEAMS
UCL > School of BEAMS > Faculty of Maths and Physical Sciences
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