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Calculation of Synthetic Ionizing Spectra for Planetary Nebulae

T. Rauch

astro-pharXiv:astro-ph/0201283

Abstract

We present a new grid (solar and halo abundance ratios) of state-of-the-art fully line-blanketed NLTE model atmospheres which covers the parameter range of central stars of planetary nebulae. The grid is available at the WWW.

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