Effects of CSPN Models on PNe Shell Modeling

Thumbnail Image

Date

Authors

Journal Title

Journal ISSN

Volume Title

Publisher

Abstract

Description

Modeling planetary nebulae (PNe) shells using different ionizing spectra for a hot central star (CSPN) of evolved PNe, we found that especially a blackbody model leads to wrong nebular diagnostics and abundances.
1 page; Proceedings of the Symposium "Ionized Gaseous Nebulae", Mexico City, 21-24 November 2000; RevMexAA (Ser. de Conf.), in press

Keywords

Astrophysics

Citation

URI

https://dspace.dare.co.zw/handle/123456789/3766

Collections

arXiv

Endorsement

Review

Supplemented By

Referenced By