Fine-Structure Transitions of Si II with Interest in Astrophysics

Details Fine-Structure Transitions of Si II with Interest in Astrophysics Fine-Structure Transitions of Si II with Interest in Astrophysics

Feb 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000apjs..126..551c&link_type=abstract

The Astrophysical Journal Supplement Series, Volume 126, Issue 2, pp. 551-559.

Astronomy and Astrophysics

Astronomy

10

Atomic Data

Scientific paper

Oscillator strengths of the dipole-allowed fine-structure transitions in Si II between the terms belonging to the 3s2nl (n=3-10) and l=0-3 configurations have been calculated in the LS-coupling scheme using the Relativistic Quantum Defect Orbital method, with and without accounting explicitly for the core-valence correlation. The present f-values are compared with other available results for this astrophysically important ion, and good agreement has been found.

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