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Quantitative Investigations on Mass Outflow from Planetary Nebulae Nuclei
Published online by Cambridge University Press: 19 July 2016
Abstract
Observed P-Cygni line profiles in the UV spectra of central stars of Planetary Nebulae (PNN) obtained with the IUE satellite has been fitted by theoretical profiles in order to determine mass loss rates.
- Type
- III. Central Stars
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- Copyright © Kluwer 1989