A comparative study between semi-empirical oscillator strength parametrization and relativistic Hartree–Fock methods for computing the radiative parameters in Zr II spectrum

Author:

Quinet P.,Bouazza S.,Palmeri P.

Funder

Scientific Research F.R.S.-FNRS

Publisher

Elsevier BV

Subject

Spectroscopy,Atomic and Molecular Physics, and Optics,Radiation

Reference23 articles.

1. Fine structure of the odd-parity Rydberg series of Zr I;Bouazza;J Phys B,2003

2. Corliss CH, Bozman WR. Experimental transition probabilities for spectral lines of seventy elements; derived from the NBS Tables of spectral-lines intensities. (NBS Monograph). US Department of Commerce, National bureau of Standards: Washington.

3. Oscillator strengths for Zr I and Zr II and a new determination of the solar abundance of zirconium;Biémont;Astrophys J,1981

4. Radiative lifetimes and transition probabilities of astrophysical interest in Zr II;Malcheva;Mon Not R Astron Soc,2006

5. New and improved experimental oscillator strengths in Zr II and the solar abundance of zirconium;Ljung;Astron Astrophys,2006

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