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An Abundance Analysis of the Silicon CP Star HD 43819
Published online by Cambridge University Press: 12 April 2016
Abstract
A fine analysis performed using four 4.3 Å/mm IIaO Mt. Wilson Observatory spectrograms shows that HD 43819 has abundance anomalies similar to those of other Silicon stars, namely it is helium, carbon, magnesium, and sulfur poor while being silicon, titanium, chromium, manganese, iron, strontium, zirconium, and rare earth rich.
- Type
- I. General Properties of CP Stars
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- Copyright © Astronomical Society of the Pacific 1993