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Emission from spherical circumstellar shells:application to Planetary Nebulae

Published online by Cambridge University Press:  08 March 2006

Ph. Stee  and
K. Gesicki
K. Gesicki*
Affiliation:
Centrum Astronomii UMK, ul. Gagarina 11, 87 100 Torun, Poland
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Abstract


Emission line spectra of planetary nebulae are computed and compared to theobservations. This allows for a derivation of the kinematical data concerningspecific nebulae as well as for general conclusions concerning stellarevolution.


Type
Research Article
Information
European Astronomical Society Publications Series , Volume 18: Radiative Transfer and Applications to Very Large Telescopes , 2006 , pp. 233 - 250
Copyright
© EAS, EDP Sciences, 2006

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