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Erratum: “Atomic Iron and Nickel in the Coma of C/1996 B2 (Hyakutake): Production Rates, Emission Mechanisms, and Possible Parents”(2021, PSJ, 2, 228)
S. J. Bromley et al 2026 The Planetary Science Journal 7 .
- Provider: AAS Journals
Caption: Figure 4.
Comparison of Ni I (left) and Fe I fluorescence models (in photon units) to the observed intensities in comet C/1965 S1 (Ikeya-Seki) as reported in C. D. Slaughter (1969) (top) and G. W. Preston (1967) (bottom). The model spectra are scaled via a linear fit of all present lines. Doppler line profiles were assumed for equilibrium temperatures derived from the heliocentric distances: 1081 K (C. D. Slaughter 1969) and 743 K (G. W. Preston 1967).
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