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Diffuse X-Ray-emitting Gas in Major Mergers

  • Authors: Beverly J. Smith, Kristen Campbell, Curtis Struck, Roberto Soria, Douglas Swartz, Macon Magno, Brianne Dunn, and Mark L. Giroux

2018 The Astronomical Journal 155 81.

  • Provider: AAS Journals

Caption: Figure 7.

Plot of the best-fit LX(gas) vs. interaction stage (open black squares), including the uncertainty in LX. The top panel gives the X-ray luminosities only corrected for Galactic absorption. The bottom panel includes internal absorption. The filled blue diamonds are the median values for each stage, slightly offset to the left. The error bars plotted on the median values are the semi-interquartile range, equal to half the difference between the 75th percentile and the 25th percentile. Upper limits above the median were not included in calculating the median. Galaxies containing a Seyfert nucleus are circled in red. The upper limits are 3σ.

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