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Stellar magnetism"

International Conference Proceedings,

1992,

233.

S i I I autoionizatio n line s an d stratifie d atmospher e i n B p typ e sta r
M . Zbori l an d J . Buda j
Astronomica l Institut e Slovak Academ y of Sciences CS-05 9 6 0 Tatrans k Lomnic a Czecho-Slovakia

Abstrac t Synthetic spectr a were computed under the assumption of atmosphere stratification for Bp type star . At 5200 depression both normal and autoionization lines strengthen at wavelengths 5187 and 5204. Lines at the former wavelength may contribute to peaked contributor of 5200 feature centered at 5175.

The complete text will appear in Lecture Notes in Physics (Springer-Verlag 1992)

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