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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 .
Caption: Figure 1.
Fluorescence spectra stick plots on a logarithmic intensity scale with the strongest lines normalized to 1 for Ni I (top) and Fe I (bottom) spanning 190–600 nm. Fluorescence efficiencies were calculated for the observing conditions of C/1996 B2 (Hyakutake), vh = −36.7 km s−1 and rh = 1.02 au.
© 2026. The Author(s). Published by the American Astronomical Society.