作者: M. Landini , B. C. M. Fossi
DOI:
关键词: Physics 、 Radiative transfer 、 Astrophysics 、 Fluorine 、 Metal ions in aqueous solution 、 Astrophysical plasma 、 Ion 、 Plasma 、 Ionization 、 Analytical chemistry 、 Autoionization
摘要: The ionization equilibrium of some cosmically less abundant elements (F, P, Cl, K, Ti, Cr, Mn and Co) is computed. computation performed using the Shull Van Steenberg (1982, Astrophys. J. Supp. Ser., 48) approximations for ionization, radiative, dielectronic autoionization rates. fitting coefficients rates are given ion abundances supplied temperatures between 10 5 8 K