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XRISM Observations of A1795: Evidence for Low Turbulence and Resonant Scattering

  • Authors: Arnab Sarkar, Eric D. Miller, Brian McNamara, Helen Russell, Kotaro Fukushima, Mark Bautz, Yutaka Fujita, Catherine E. Grant, François Mernier, Michael A. McDonald, Naomi Ota, Ayşegül Tümer, Daniel Wik

Arnab Sarkar et al 2026 The Astrophysical Journal Letters 1005 .

  • Provider: AAS Journals

Caption: Figure 2.

Left panels: XRISM/Resolve subarray counts spectra are shown along with the best-fit 1T models after accounting for spatial–spectral mixing. In all four panels, the best-fit model components are folded through the relevant instrumental response and plotted as follows: red, blue, green, orange, purple, magenta, and cyan for the total model, region 1 (0–0﹩\mathop{.}\limits^{{\rm{^{\prime} }}}﹩75), region 2 (0﹩\mathop{.}\limits^{{\rm{^{\prime} }}}﹩75–1﹩\mathop{.}\limits^{{\rm{^{\prime} }}}﹩5), region 3 (1﹩\mathop{.}\limits^{{\rm{^{\prime} }}}﹩5–3﹩{}^{{\prime} }﹩), region 4 (3﹩{}^{{\prime} }﹩–4﹩\mathop{.}\limits^{{\rm{^{\prime} }}}﹩5), NXB, and CXB, respectively. Bottom panels in all four spectra represent ratios between data/model. Right panels: same as left but zoomed into Fe xxv-Heα and Fe xxvi-Lyα line complexes.

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