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.
Author details: | Jiří KubátORCiD, S. M. Saad |
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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): | Keine 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 |