Moving absorption bumps in the spectra of Be stars

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.

Bibliographic Details
Main Authors: Kubát, J., Saad, S. M.
Format: Others
Language:English
Published: Universität Potsdam 2007
Subjects:
Online Access:http://nbn-resolving.de/urn:nbn:de:kobv:517-opus-17879
http://opus.kobv.de/ubp/volltexte/2008/1787/