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Emission from spherical circumstellar shells: application to Planetary Nebulae
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Radiative Transfer and Applications to Very Large Telescopes
Title
Emission from spherical circumstellar shells: application to Planetary Nebulae
Date
2006-01-01
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http://hub.abes.fr/edp/periodical/eas/2006/volume_18/issue_2006/eas18014/m/print
http://hub.abes.fr/edp/periodical/eas/2006/volume_18/issue_2006/eas18014/m/web
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http://hub.abes.fr/edp/periodical/eas/2006/volume_18/issue_2006/eas18014/authorship/2
http://hub.abes.fr/edp/periodical/eas/2006/volume_18/issue_2006/eas18014/authorship/1
Author
Gesicki, K.
Editor
Stee, Ph.
Abstract
Emission line spectra of planetary nebulae are computed and compared to the observations. This allows for a derivation of the kinematical data concerning specific nebulae as well as for general conclusions concerning stellar evolution.
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eas18014
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2006-01-01
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© EAS, EDP Sciences, 2006
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