Hostname: page-component-586b7cd67f-vdxz6 Total loading time: 0 Render date: 2024-11-26T15:03:45.093Z Has data issue: false hasContentIssue false

MBPT Results for Δn=0 Electric Dipole Transitions

Published online by Cambridge University Press:  07 August 2017

G. Gaigalas
Affiliation:
Institute of Theoretical Physics and Astronomy, Gostauto 12, 2600, Vilnius, Lithuania
R. Kisielius
Affiliation:
Institute of Theoretical Physics and Astronomy, Gostauto 12, 2600, Vilnius, Lithuania
G. Merkelis
Affiliation:
Institute of Theoretical Physics and Astronomy, Gostauto 12, 2600, Vilnius, Lithuania
Z. Rudzikas
Affiliation:
Institute of Theoretical Physics and Astronomy, Gostauto 12, 2600, Vilnius, Lithuania
M. Vilkas
Affiliation:
Institute of Theoretical Physics and Astronomy, Gostauto 12, 2600, Vilnius, Lithuania

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

To identify spectra of Planetary Nebulae which usually have many atomic lines one needs very accurate theoretical atomic data.

Type
II. Highlights on the Nuclei
Copyright
Copyright © Kluwer 1993 

References

1. Vilkas, M.J., Gaigalas, G., Merkelis, G. 1991, Lithuanian J. Phys., 31, 84 Google Scholar
2. Flaig, H.J., Schartner, K.-H., Trabert, E., Heckmann, P.H., 1985, Physica Scripta, 31, 225 Google Scholar
3. Baluja, K.L., Zeippen, C.J., 1989, J. Phys. B, 21, 15 Google Scholar
4. Cheng, K.T., Kim, J.K., Desclaux, J.P., 1979, At. Data Nucl. Data Tables, 24, 111 Google Scholar