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.

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Author details:Jiří KubátORCiD, S. M. Saad
URN:urn:nbn:de:kobv:517-opus-17879
Publication type:Conference Proceeding
Language:English
Publication year:2007
Publishing institution:Universität Potsdam
Release date:2008/04/25
RVK - Regensburg classification:US 1999.07
Organizational units:Extern / Extern
DDC classification:5 Naturwissenschaften und Mathematik / 52 Astronomie / 520 Astronomie und zugeordnete Wissenschaften
Collection(s):Universität Potsdam / Tagungsbände/Proceedings (nicht fortlaufend) / Clumping in hot-star winds: International Workshop, Potsdam, Germany, 18. - 22. June 2007
Universität Potsdam / Tagungsbände/Proceedings (nicht fortlaufend) / Clumping in hot-star winds: International Workshop, Potsdam, Germany, 18. - 22. June 2007 / Posters
License (German):License LogoKeine öffentliche Lizenz: Unter Urheberrechtsschutz
External remark:
The complete edition of the proceedings "Clumping in hot-star winds" is available:
urn:nbn:de:kobv:517-opus-13981
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