Keywords
Be Stars: UV Spectroscopy
Be Stars: Circumstellar Shells
Be Stars: Metal Lines
Circumstellar Shells: Rotation
Be Stars: Circumstellar Shells
Be Stars: Metal Lines
Circumstellar Shells: Rotation
How to Cite
Spectroscopic analysis of 48 Lib in the ultraviolet range. (1990). Revista Mexicana De Astronomía Y Astrofísica, 21(1), 424. https://astronomia.unam.mx/journals/rmxaa/article/view/1990rmxaa..21..424l
Abstract
To determine the physical conditions of the gaseous envelope of this star the authors analyze its spectrum in the ultraviolet range (λ1250 - 3100 Å) on the basis of the data supplied by the International Ultraviolet Explorer satellite (IUE). The results show that the envelope has a small rotational speed. In this envelope the narrow and deep lines of Fe II, Ni II, and Ti III are originated. In a deeper thin region that rotates with the star the lines of Al III and - apparently - of Si IV are present. These lines show broad profiles due to a high rotational speed.Similar Articles
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