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- W1976097225 abstract "It is suggested that if early-type Beta Cephei variables are pulsating nonradially, then electron scattering should produce a varying net polarization. This should be observable in at least some stars in the near or far UV. Computations are presented which show that for BW Vul the total amplitude may be as great as 0.03%. An observing program is proposed." @default.
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- W1976097225 date "1979-06-01" @default.
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- W1976097225 title "Possible polarization effects in the Beta Cephei stars" @default.
- W1976097225 doi "https://doi.org/10.1086/130492" @default.
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