Properties of Regions Forming the FeII Emission Lines in Be Stars
classification
🌌 astro-ph
keywords
emissionfeiilinesformingpropertiesregionsstarsbalmer
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We study FeII and Balmer hydrogen emission lines observed simultaneously of 18 southern Be stars. We use the self-absorption-curve method (SAC) to determine the optical depth regime of FeII emission lines and to derive first insights on the physical properties of their forming regions.
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