Effects of CSPN Models on PNe Shell Modeling
Astrophysics
2007-05-23 v1
Abstract
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.
Keywords
Cite
@article{arxiv.astro-ph/0106266,
title = {Effects of CSPN Models on PNe Shell Modeling},
author = {B. Armsdorfer and S. Kimeswenger and T. Rauch},
journal= {arXiv preprint arXiv:astro-ph/0106266},
year = {2007}
}
Comments
1 page; Proceedings of the Symposium "Ionized Gaseous Nebulae", Mexico City, 21-24 November 2000; RevMexAA (Ser. de Conf.), in press