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- W4230778984 abstract "It is a good tradition in IAU Symposia about PN to have a paper on model atmospheres. However, this is always a difficult task for the authors, because the majority of the PN researchers still believe that the best model atmosphere for a Central Star is a black body. Of course, this puts a theorist in stellar atmospheres into a somewhat desperate position. However, Central Stars of Planetary Nebulae (hereafter CSPN) - as all other stars - show spectral lines. And we will try to use the opportunity of this paper to convince that - as for all other stars - the quantitative analysis of these lines on basis of model atmospheres yields extremely valuable information about the physical nature of the stars." @default.
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- W4230778984 date "1989-01-01" @default.
- W4230778984 modified "2023-09-26" @default.
- W4230778984 title "Model Atmospheres and Quantitative Spectroscopy of Central Stars of Planetary Nebulae" @default.
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- W4230778984 doi "https://doi.org/10.1017/s007418090013846x" @default.
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