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- W297835844 abstract "On presente un modele qui suppose un mouvement vers l'exterieur des filaments emetteurs dans un milieu dilue. Les effets du front de choc et d'une source de rayonnement centrale agissent sur les bords opposes des filaments isoles. Les resultats deduits du modele confirment l'existence de deux types de noyaux galactiques actifs suivant qu'ils sont domines par le choc ou par le rayonnement" @default.
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- W297835844 date "1985-08-01" @default.
- W297835844 modified "2023-09-28" @default.
- W297835844 title "Composite models for the narrow emission line region of active galactic nuclei. III: The ejected filament" @default.
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