ATOMIC DATA AND SPECTRAL MODEL FOR Fe III

作者：Bautista Manuel A^*; Ballance Connor P; Quinet Pascal

来源：Astrophysical Journal Letters, 2010, 718(2): L189-L193.

DOI：10.1088/2041-8205/718/2/L189

• atomic data
• circumstellar matter
• H II regions
• ISM: atoms
• quasars: absorption lines
• quasars: emission lines

We present new atomic data (radiative transitions rates and collision strengths) from large-scale calculations and a non-LTE spectral model for Fe III. This model is in very good agreement with observed astronomical emission spectra, in contrast with previous models that yield large discrepancies in observations. The present atomic computations employ a combination of atomic physics methods, e.g., relativistic Hartree-Fock, the Thomas-Fermi-Dirac potential, and Dirac-Fock computation of A-values and the R-matrix with intermediate coupling frame transformation and the Dirac R-matrix. We study advantages and shortcomings of each method. It is found that the Dirac R-matrix collision strengths yield excellent agreement with observations, much improved over previously available models. By contrast, the transformation of the LS-coupling R-matrix fails to yield accurate effective collision strengths at around 104 K, despite using very large configuration expansions, due to the limited treatment of spin-orbit effects in the near-threshold resonances of the collision strengths. The present work demonstrates that accurate atomic data for low-ionization iron-peak species are now within reach.

• 出版日期2010-8-1