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Stark broadened line profiles of neutral strontium lines in plasma conditions

Published online by Cambridge University Press:  25 May 2016

Milan S. Dimitrijević  and
Sylvie Sahal-Bréchot
Milan S. Dimitrijević
Affiliation:
1Astronomical Observatory, Volgina 7, 11050 Belgrade, Serbia, Yugoslavia
Sylvie Sahal-Bréchot
Affiliation:
2Observatoire de Paris–Meudon, 92190 Meudon, France

Extract

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During more than twenty years, we are making a continuous effort to provide Stark-broadening parameters needed for research of astrophysical, laboratory and laser produced plasma. A review of our results is presented in Dimitrijević, 1996). Such data are of interest for the consideration of a number of problems in astrophysics, physics and technology as e.g. for stellar plasma diagnostic, opacity calculations, the investigation/modelling of stellar spectra or a particular line, laboratory plasma diagnostic, laser produced plasmas, thermonuclear research, plasma technology, as well as for different examinations of regularities and systematic trends for e.g. homologous atoms (Dimitrijević and Popović, 1989) or in general (Purić et al. 1991).

Type
IV. Envelopes
Information
Symposium - International Astronomical Union , Volume 180: Planetary Nebulae , 1997 , pp. 219
Copyright
Copyright © Kluwer 1997 

References

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