Line Profile microvariability and wind structure for OB stars

Details Line Profile microvariability and wind structure for OB stars Line Profile microvariability and wind structure for OB stars

Jul 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011iaus..272..200k&link_type=abstract

Active OB stars: structure, evolution, mass loss, and critical limits, Proceedings of the International Astronomical Union, IAU

Other

Stars: Early-Type, Stars: Variables: Other, Line: Profiles, Stars: Winds, Outflows

Scientific paper

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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