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- W1544943670 abstract "We present new UBVRI observations of the magnetic Bp star sigma Ori E. The basic features of the star's lightcurve have not changed since the previous monitoring by Hesser et al. (1977), indicating that the star's magnetosphere has remained stable over the past three decades. Interestingly, we find a rotation period that is slightly longer than in the Hesser et al. (1977) analysis, suggesting possible spindown of the star." @default.
- W1544943670 created "2016-06-24" @default.
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- W1544943670 date "2005-11-15" @default.
- W1544943670 modified "2023-09-27" @default.
- W1544943670 title "New Photometric Observations of sigma Ori E" @default.
- W1544943670 hasPublicationYear "2005" @default.
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