SIMBAD references

2018ApJS..234...40W - Astrophys. J., Suppl. Ser., 234, 40-40 (2018/February-0)

Benchmarking atomic data for astrophysics: Be-like ions between B II and Ne VII.

WANG K., CHEN Z.B., ZHANG C.Y., SI R., JONSSON P., HARTMAN H., GU M.F., CHEN C.Y. and YAN J.

Abstract (from CDS):

Large-scale self-consistent multiconfiguration Dirac-Hartree-Fock and relativistic configuration interaction calculations are reported for the n≤ 6 levels in Be-like ions from B II to Ne VII. Effects from electron correlation are taken into account by means of large expansions in terms of a basis of configuration state functions, and a complete and accurate data set of excitation energies; lifetimes; wavelengths; electric dipole, magnetic dipole, electric quadrupole, and magnetic quadrupole line strengths; transition rates; and oscillator strengths for these levels is provided for each ion. Comparisons are made with available experimental and theoretical results. The uncertainty of excitation energies is assessed to be 0.01% on average, which makes it possible to find and rule out misidentifications and aid new line identifications involving high-lying levels in astrophysical spectra. The complete data set is also useful for modeling and diagnosing astrophysical plasmas.

Abstract Copyright: © 2018. The American Astronomical Society. All rights reserved.

Journal keyword(s): atomic data - atomic processes

VizieR on-line data: <Available at CDS (J/ApJS/234/40): table1.dat table5.dat>

Simbad objects: 4

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