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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 11.

Top panel: diffuse LX(gas)/LFIR, after only correcting for Galactic absorption, plotted vs. SFR. The data points are color-coded by merger stage. Merger stages 1 and 2 systems are marked as open green triangles. Merger stages 3, 4, and 5 are open cyan diamonds, and merger stages 6 and 7 are identified by blue open squares. Galaxies containing a Seyfert nucleus are circled in red. Black crosses mark the normal spirals from Mineo et al. (2012b). Middle panel: plot of diffuse LX(gas)/SFR vs. SFR, where the X-ray is only corrected for Galactic absorption. Bottom panel: plot of diffuse LX(gas)/SFR vs. SFR, after correction for internal absorption.

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