A multi-wavelength study of fast winds from central stars of planetary nebulae
Structure has been observed in the stellar outflows of hot, luminous OB stars through the temporal spectral analysis of UV data: the absorption troughs of wind-accelerated P-Cygni profiles of certain UV ‘super-ions’, particularly the Pv λλ 1118, 1128 doublet, have revealed the presence of additional...
| Main Author: | |
|---|---|
| Published: |
University College London (University of London)
2012
|
| Subjects: | |
| Online Access: | http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.565635 |