Hostname: page-component-586b7cd67f-l7hp2 Total loading time: 0 Render date: 2024-11-26T03:44:22.744Z Has data issue: false hasContentIssue false
  • English
  • Français

MBPT Results for Δn=0 Electric Dipole Transitions

Published online by Cambridge University Press:  07 August 2017

G. Gaigalas ,
R. Kisielius ,
G. Merkelis ,
Z. Rudzikas  and
M. Vilkas
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
Information
Symposium - International Astronomical Union , Volume 155: Planetary Nebulae , 1993 , pp. 96
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