Search

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation
Large resolution
Hi-Resolution Export to PDF

Atomic Iron and Nickel in the Coma of C/1996 B2 (Hyakutake): Production Rates, Emission Mechanisms, and Possible Parents

  • Authors: S. J. Bromley, B. Neff, S. D. Loch, J. P. Marler, J. Országh, K. Venkataramani, D. Bodewits

S. J. Bromley et al 2021 The Planetary Science Journal 2 .

  • Provider: AAS Journals

Caption: Figure 7.

Comparison of modeled and observed line intensities of Ni I (left) and Fe I (right). Model error bars are taken as the quadrature sum of the Monte Carlo uncertainty and the sensitivity to heliocentric velocity (see text), and an absolute error for the observed intensities was assumed to be ±40% (Meier et al. 1998).

Other Images in This Article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Copyright and Terms & Conditions

Additional terms of reuse