Effects of CSPN Models on PNe Shell Modeling

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dc.creatorArmsdorfer, B.
dc.creatorKimeswenger, S.
dc.creatorRauch, T.
dc.date2001-06-14
dc.date.accessioned2026-07-07T01:58:55Z
dc.date.available2026-07-07T01:58:55Z
dc.descriptionModeling 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.
dc.description1 page; Proceedings of the Symposium "Ionized Gaseous Nebulae", Mexico City, 21-24 November 2000; RevMexAA (Ser. de Conf.), in press
dc.identifierhttps://arxiv.org/abs/astro-ph/0106266
dc.identifierhttp://arxiv.org/abs/astro-ph/0106266
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/2907
dc.subjectAstrophysics
dc.titleEffects of CSPN Models on PNe Shell Modeling
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