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Non-LTE Model Atmosphere Analysis of Central Stars

  • R.H. Méndez (a1) (a2) (a3), R. P. Kudritzki (a4) and K. P. Simon (a4)

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This review will be concentrated on the determination of the main atmospheric parameters (Teff, log g, helium abundance) of PN nuclei, and of other subluminous objects, by fitting the observed absorption line profiles with theoretical profiles obtained from non-LTE model atmosphere calculations.

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References

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Non-LTE Model Atmosphere Analysis of Central Stars

  • R.H. Méndez (a1) (a2) (a3), R. P. Kudritzki (a4) and K. P. Simon (a4)

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