UV and soft X-ray observations of central stars of planetary nebulae and hot white dwarfs
The first IUE SWP high-resolution spectral atlas of central stars of planetary nebulae and hot white dwarfs is presented. Its primary aim is as a set of comparison spectra, with which it is shown that LS V +46 21, the postulated central star of S 216, has a temperature Teff = 80, 000K + 10,000K, and...
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University of Leicester
1991
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| Online Access: | https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.737367 |