MOST Observations of σ Ori E: Challenging the Centrifugal Breakout Narrative
The Astrophysical Journal, Volume 769, Issue 1, article id. 33, 5 pp. (2013).
Published in May 2013
We present results from three weeks' photometric monitoring of the magnetic helium-strong star σ Ori E using the Microvariability and Oscillations of Stars microsatellite. The star's light curve is dominated by twice-per-rotation eclipse-like dimmings arising when magnetospheric clouds transit across and occult the stellar disk. However, no evidence is found for any abrupt centrifugal breakout of plasma from the magnetosphere, either in the residual flux or in the depths of the light minima. Motivated by this finding we compare the observationally inferred magnetospheric mass against that predicted by a breakout analysis. The large discrepancy between the values leads us to argue that centrifugal breakout does not play a significant role in establishing the magnetospheric mass budget of σ Ori E.
Astrophysics - Solar and Stellar Astrophysics; circumstellar matter; stars: chemically peculiar; stars: early-type; stars: individual: HD 37479; stars: magnetic field; stars: rotation
circumstellar matter; stars: chemically peculiar; stars: early-type; stars: individual: HD 37479; stars: magnetic field; stars: rotation
Astrophysics - Solar and Stellar Astrophysics