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UV Observations of Three Classical Novae during Early Stages of Decline*
Published online by Cambridge University Press: 12 April 2016
Abstract
We present IUE UV spectra of the three recent classical novae N Sgr 1982, N Ser 1983, and N Mus 1983, obtained during early decline, transitional stage, and nebular phase, respectively. The line spectra are discussed. Preliminary conclusions concerning CNO over-abundances, shell geometry, and speed classes are drawn.
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- Research Article
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- Copyright
- Copyright © Reidel 1984
Footnotes
Paper presented at the Lembang-Bamberg 1AU Colloquium No. 80 on ‘Double Stars: Physical Properties and Generic Relations', held at Bandung, Indonesia, 3-7 June, 1983.