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- W289127222 abstract "On suggere que dans le coeur radiatif d'etoiles de type solaire, un champ magnetique complique de quelques milliers de Gauss (pour K=10 −7 cm −1 ) avec un spectre B (K)=const.K −1/3 est maintenu" @default.
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- W289127222 date "1986-11-01" @default.
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- W289127222 title "Is it possible to maintain magnetic fields in the radiative cores of rotating stars with convective envelopes" @default.
- W289127222 hasPublicationYear "1986" @default.
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