Abstract
A high-resolution IUE spectral atlas of central stars of planetary nebulae and hot white dwarfs has been produced (part of Tweedy, 1991, PhD thesis from the University of Leicester, UK), and examples from it are shown here. It has been sorted into an approximate evolutionary sequence, based on published spectroscopic analyses, from the cool 28,000K young central star He 2–138, through the hot objects like NGC 7293 and NGC 246 at 90,000K and 130,000K respectively, down to 40,000K DA white dwarfs like GD 2, which is the chosen cutoff for this selection. Copies of a revised version of this atlas, which will include more recent spectroscopic information and also white dwarfs down to 35,000K - to include the Si III object GD 394 - will be sent to anyone who requests one.
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© 1993 Springer Science+Business Media Dordrecht
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Tweedy, R.W. (1993). A High Resolution Far-UV Spectral Atlas of CSPNs and Hot White Dwarfs. In: Weinberger, R., Acker, A. (eds) Planetary Nebulae. International Astronomical Union / Union Astronomique Internationale, vol 155. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-2088-3_31
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DOI: https://doi.org/10.1007/978-94-011-2088-3_31
Publisher Name: Springer, Dordrecht
Print ISBN: 978-0-7923-2440-9
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