Model Atmospheres and Quantitative Spectroscopy of Central Stars of Planetary Nebulae
1989 ◽
Vol 131
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pp. 273-292
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Keyword(s):
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.
1989 ◽
Vol 131
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pp. 355-355
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Keyword(s):
1989 ◽
Vol 131
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pp. 411-424
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Keyword(s):
1997 ◽
Vol 180
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pp. 269-269
Keyword(s):
1997 ◽
Vol 180
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pp. 287-287
Keyword(s):
1983 ◽
Vol 103
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pp. 230-230
2003 ◽
Vol 209
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pp. 541-542
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Keyword(s):