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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. |
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