Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientific paper
2010-09-17
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
2 pages, 1 figure, IAUS 272 - Active OB Stars: Structure, Evolution, Mass Loss and Critical Limits
Scientific paper
A magnetic field and rotational line profile variability (lpv) is found in
the He-weak star HR2949. The field measured from metallic lines varies in a
clearly non-sinusoidal way, and shows a phase lag relative to the
morphologically similar HeI equivalent width variations. The surface abundance
patterns are strong and complex, and visible even in the hydrogen lines.
Grunhut Jason
Rivinius Th.
Shultz Matt
Stahl Otmar
the MiMeS Collaboration
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