A model for the origin of the anomalous and very bright UV lines of Fe II in gaseous condensations of the star $\mathsf{\eta}$ Carinae

Publisher： Edp Sciences

E-ISSN： 1432-0746|378|1|266-278

ISSN： 0004-6361

Source： Astronomy & Astrophysics, Vol.378, Iss.1, 2001-10, pp. : 266-278

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