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Be Envelope Properties Determined from Fe II Emission Lines1
Published online by Cambridge University Press: 12 April 2016
Abstract
Applying the SAC (self absorption curve) method to χ Oph (HD 148184) we conclude that Fell emission lines are optically thick. We estimate the excitation temperature of the permitted Fe II line formation region and the dimensions of this region. We conclude that this region may possibly have a non-uniform density structure.
- Type
- 6. Disks
- Information
- International Astronomical Union Colloquium , Volume 175: The Be Phenomenon in Early-Type Stars , 2000 , pp. 523 - 526
- Copyright
- Copyright © Astronomical Society of the Pacific 2000
Footnotes
Data obtained in CASLEO operated under agreement between the CONICET and the Universities of La Plata, Córdoba and San Juan - Argentina
References
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