Effects of CSPN Models on PNe Shell Modeling
classification
🌌 astro-ph
keywords
cspnmodelingabundancesblackbodycentraldiagnosticsdifferenteffects
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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.
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