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- W1639568613 abstract "On explique generalement le flux de RX mou observe dans Sirius B par l'existence d'un flux acoustique, de l'ordre de 10 29 erg s −1 , genere dans la zone convective sub-photospherique. On developpe une hypothese alternative de generation du flux acoustique suivant le fait que les modeles d'enveloppe a couches de cette etoile sont instables aux oscillations de courte periode (0,06 a 0,45 s) si la couche riche en hydrogene est suffisamment peu profonde. On suggere que le flux acoustique est genere par l'interaction resonantes a phase quelconque entre les modes instables et les ondes itinerantes" @default.
- W1639568613 created "2016-06-24" @default.
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- W1639568613 date "1983-01-01" @default.
- W1639568613 modified "2023-10-17" @default.
- W1639568613 title "On the origin of the acoustic flux in Sirius B" @default.
- W1639568613 hasPublicationYear "1983" @default.
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