Stark broadening of Ca I Virtual Observatory Resource

Authors

1. Dimitrijevic M.S.
2. Sahal-Brechot S.

Published by

CDS

Abstract

Using the semiclassical perturbation approach, we have calculated electron-, proton-, He II-, Mg II-, Si II- and Fe II-impact line widths and shifts for 189 Ca I multiplets as a function of temperature and perturber density. Perturbers selected here are the main perturbers in solar atmospheres. Obtained results have been compared with the existing theoretical and experimental data.

Keywords

1. Atomic physics

Bibliographic source Bibcode

1999A&AS..140..191D

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+AS/140/191

IVOA Identifier IVOID

ivo://CDS.VizieR/J/A+AS/140/191

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Web browser access HTML

http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+AS/140/191
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+AS/140/191
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+AS/140/191

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