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Elemental Abundances in the Diffuse Interstellar Medium from Joint Far-ultraviolet and X-Ray Spectroscopy: Iron, Oxygen, Carbon, and Sulfur

  • Authors: I. Psaradaki, L. Corrales, J. Werk, A. G. Jensen, E. Costantini, M. Mehdipour, R. Cilley, N. Schulz, J. Kaastra, J. A. García, L. Valencic, T. Kallman, F. Paerels

I. Psaradaki et al 2024 The Astronomical Journal 167 .

  • Provider: AAS Journals

Caption: Figure 7.

Comparison of the literature standard abundance tables of Fe, O, and S with the values of this work derived from FUV and X-ray observations presented in Table 5. The log(O/Ne) ratio is the sum of the predicted O I abundance that we obtain from a simultaneous X-ray and FUV fit and the solid-phase oxygen. For the log(Fe/Ne) ratio, we used the combined contribution of solid iron and atomic Fe II. Please note that the log(S/Ne) ratio comes from the S II value only resulting from the FUV fit. The Ne abundance is determined through the fit of the Ne K-edge in the X-ray spectrum from Psaradaki et al. (2023); in particular, it represents the summed abundance of Ne I, Ne II, and Ne III.

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