Refine
Has Fulltext
- yes (246) (remove)
Year of publication
Document Type
- Conference Proceeding (246) (remove)
Language
- English (186)
- German (49)
- Multiple languages (10)
- French (1)
Keywords
- Archiv (4)
- Information Structure (4)
- Nachlass (4)
- Cloud Computing (3)
- E-Learning (3)
- middleware (3)
- Constraint Solving (2)
- Deduction (2)
- EMOTIKON (2)
- Forschungsprojekte (2)
Institute
- Extern (137)
- Interdisziplinäres Zentrum für Musterdynamik und Angewandte Fernerkundung (23)
- Institut für Künste und Medien (20)
- Institut für Informatik und Computational Science (15)
- Institut für Slavistik (14)
- Institut für Physik und Astronomie (11)
- Institut für Geowissenschaften (10)
- Hasso-Plattner-Institut für Digital Engineering gGmbH (9)
- Sonderforschungsbereich 632 - Informationsstruktur (7)
- Bürgerliches Recht (6)
Hα observations of Rigel obtained on 184 nights during the past ten years with the 1-m telescope and ´echelle spectrograph of Ritter Observatory are surveyed. The line profiles were classified in terms of morphology. About 1/4 of them are of P Cygni type, about 15% inverse P Cygni, about 25% double-peaked, about 1/3 pure absorption, and a few are single emission lines. Transformation of the profile from one type to another typically takes a few days. Although the line stays in absorption for extended intervals, only one high-velocity absorption event of the intensity reported by Kaufer et al. (1996a) was observed, in late 2006. Late in this event, Hα absorption occurred farther to the red than the red wing of a plausible photospheric absorption component, an indication of infalling material. In general, as the absorption events come to an end, the emission typically returns with an inverse P Cygni profile. The Hα profile class shows no obvious correlation with the radial velocity of C II λ6578, a photospheric absorption line.