Abstract:Ten lines in the range 3880;:; A ::a 5666 A in the beam-foil spectrum of iron have been identified with specific hydrogenic transitions in Fe rv-vxu. The same transitions were observed from Ni and Ar beams. Deviations from the hydrogenic wavelengths are shown to be consistent with that expected from core polarization. The absence of these lines in astrophysical sources is discussed. A wavelength table is presented for identificat!lon of hydrogenic transitions to be expected in beam-foil spectra.
“…numbers are as high as 15 and even 16. This agrees with the observation by Lennard et al [24], that the only limit for observation of these transitions is the long wavelength limit of the instrument. In this connection it is noteworthy that no An=3 transitions with n > 15 have been seen within the observable wavelength region.…”
“…numbers are as high as 15 and even 16. This agrees with the observation by Lennard et al [24], that the only limit for observation of these transitions is the long wavelength limit of the instrument. In this connection it is noteworthy that no An=3 transitions with n > 15 have been seen within the observable wavelength region.…”
“…Hallin et al [2] further observed many such lines belonging to ClVI -CIXIV. It is worth adding that in a beam-foil experiment on Fe and Ni, Lennard et al [9] observed previously unreported hydrogen-like transitions in FeIV -FeVIII and NiIV -NiVIII.…”
“…The data are shown in Table 7, and are plotted in Figs. [43][44][45][46][47][48]. Although polarization apparently varies as a function of energy (59), a polarization change from 5% to 20% would results in only a 2% change in the correction fac tor.…”
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