Moving absorption bumps in the spectra of Be stars

Details Moving absorption bumps in the spectra of Be stars Moving absorption bumps in the spectra of Be stars

Apr 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008cihw.conf..245k&link_type=abstract

Clumping in hot-star winds : proceedings of an international workshop held in Potsdam, Germany, 18. - 22. June 2007. Hamann, Wol

Physics

Scientific paper

Several Be binaries exhibit an absorption bump moving across the blue
wing of hydrogen emission lines towards the line center. This bump is
demonstrated for the case of two bright Be stars, κ Dra and 4 Her.
It is not clear what is the reason for this travelling bump.

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