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- W16103469 abstract "Differential UBV photometry of the southern helimu-strong star HD 96446 collectd in 1987 and 1990 at two observatories reveals periodic light variations with a V amplitude of ∼ 0.02 mag. The period which best satisfies both these data and the available magnetic observations is 0.85137 d. If these variations are due to rotational modulation in a magnetic oblique rotator, this would make HD 96446 one of the most rapidly rotating He-strong stars known, despite a v sin i ≤ 16 km/s." @default.
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- W16103469 date "1991-03-01" @default.
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- W16103469 title "The helium-strong star HD 96446 : a rapid rotator and possible pulsator?" @default.
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