NASA NTRS · 19850009456
Active Phenomena in the Pre-main Sequence Star AB AUR
Abstract
The Herbig Ae star AB Aur presents short time scale variability in the Mg II and Ca II resonance lines. A qualitative model of the expanding envelope, involving fast and slow streams in a co-rotating structure, is proposed to explain the Mg II spectral variability.
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Praderie, F., Simon, T., Boesgaard, A. M., Felenbok, P., Catala, C., Czarny, J., Talavera, A.. 1985-01-01. Active Phenomena in the Pre-main Sequence Star AB AUR. https://ntrs.nasa.gov/citations/19850009456
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