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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 5.

Posterior distribution for the simultaneous FUV and X-ray spectrum in the oxygen region. The distribution compares each pair of free parameters of the fit with two-dimensional histograms. The parameters in the plot correspond to the following quantities: N H is the neutral hydrogen column density in units of 1021 cm−2 along the line of sight; z v is the velocity shift in km s−1; ﹩\mathrm{log}({\mathrm{norm}}_{\mathrm{bb}})﹩ is the logarithm of the blackbody normalization; N dust is the total column density of dust in 1018 cm−2; b refers to the line velocity broadening in km s−1; O II, O III, and O IV correspond to the logarithmic ionic column densities in cm−2; and Oabund is the O abundance scale factor relative to Lodders & Palme (2009).

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