Ionization-correction factors for the chemical composition determination of planetary nebulae with density gas fluctuations taking into account

270 photo ionization models of planetary nebulae luminescence was calculated. Free parameters for the models grid were energy distribution at the wavelengths 6912˚A, filling factor and chemical composition. T∗ and r∗ in models were selected from Blocker’s evolutional tracks. Energy distributions in...

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Bibliographic Details
Main Author: N. V. Gavrilova
Format: Article
Language:English
Published: National Aviation University 2003-12-01
Series:Вісник Астрономічної школи
Online Access:http://astro.nau.edu.ua/issues/2003_V.4_Iss.2/099.html