Active phenomena in the pre-main sequence star AB AUR

Details Active phenomena in the pre-main sequence star AB AUR Active phenomena in the pre-main sequence star AB AUR

Jan 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985nascp2358...81p&link_type=abstract

In NASA. Goddard Space Flight Center The Origin of Nonradiative Heating/Momentum in Hot Stars p 81-85 (SEE N85-17755 08-88)

Physics

Pre-Main Sequence Stars, Stellar Envelopes, Stellar Models, Calcium, Iue, Magnesium, Resonance Lines, Stellar Spectra, Variability

Scientific paper

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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