| DOI | Resolve DOI: https://doi.org/10.1088/0004-637X/769/1/33 |
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| Author | Search for: Townsend, R. H. D.; Search for: Rivinius, Th.; Search for: Rowe, J. F.; Search for: Moffat, A. F. J.; Search for: Matthews, J. M.; Search for: Bohlender, D.1; Search for: Neiner, C.; Search for: Telting, J. H.; Search for: Guenther, D. B.; Search for: Kallinger, T.; Search for: Kuschnig, R.; Search for: Rucinski, S. M.; Search for: Sasselov, D.; Search for: Weiss, W. W. |
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| Affiliation | - National Research Council of Canada. National Science Infrastructure
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| Format | Text, Article |
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| Abstract | 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. |
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| Publication date | 2013-05-02 |
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| In | |
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| Language | English |
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| Peer reviewed | Yes |
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| NPARC number | 21270383 |
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| Export citation | Export as RIS |
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| Report a correction | Report a correction (opens in a new tab) |
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| Record identifier | c468f727-442d-4511-b474-bfc4e98968e2 |
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| Record created | 2014-02-06 |
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| Record modified | 2020-04-22 |
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