Back to Volume
Paper: Structure of WNE Wolf-Rayet stars as derived from the Fe V and Fe VI pseudocontinua
Volume: 7, Properties of Hot Luminous Stars: Boulder-Munich Workshop
Page: 139
Authors: Koenigsberger, Gloria
Abstract: From phase-dependent variations in the Fe V and Fe VI pseudocontinua in four WNE+O binary systems, the ionization structure described by the ratio of Fe VI/Fe V is found. The effect of selective 'extinction' due to the WR star's wind on the WR's core is derived empirically, allowing for a correction to the 1200 - 2000 A continuum distribution.
Back to Volume