The spectral line synthesis study in Belgrade.

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Plasma: Solar Atmosphere, Plasma: Stellar Atmospheres

Scientific paper

Investigation of both solar and stellar atmospheres using the spectral line synthesis method in the astrophysical group of the Belgrade Observatory started in 1983. The study of the pressure broadening in the astrophysical plasma and related topics are the main research orientation. Corresponding computer programs are developed. A review of the first results and the current investigations concerning line asymmetries and shifts caused by pressure, abundance determinations and microturbulence is given.

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