Hostname: page-component-78c5997874-4rdpn Total loading time: 0 Render date: 2024-11-04T19:30:32.437Z Has data issue: false hasContentIssue false
  • English
  • Français

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
Get access

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

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)