Quantitative Investigations on Mass Outflow from Planetary Nebulae Nuclei

S. Cerrato, L. Bianchi,M. Grewing,M. Bässgen,G. Bässgen

Symposium（1989）

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摘要

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.

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