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XRISM Observations of the Prototypical Cold Front in A3667

  • Authors: Yuki Omiya, Yuto Ichinohe, Kazuhiro Nakazawa, Hisamitsu Awaki, Dominique Eckert, Yutaka Fujita, Isamu Hatsukade, Maxim Markevitch, François Mernier, Ikuyuki Mitsuishi, Naomi Ota, Aurora Simionescu, Yuusuke Uchida, Shutaro Ueda, Irina Zhuravleva, John Zuhone

Yuki Omiya et al 2026 The Astrophysical Journal Letters 996 .

  • Provider: AAS Journals

Caption: Figure 6.

Data-to-model ratio plots corresponding to the spectral fits shown in Figure 2. Alt text: Ten line graphs. In the upper left panel, the x-axis shows the energy from 2.0 to 10.0 keV. The y-axis shows the data-to-model ratio from 0 to 4. In the upper right panel, the x-axis shows the energy from 6.2 to 6.7 keV. The y-axis shows the data-to-model ratio from 0 to 4. In the second row of panels, the x-axis shows the energy from 6.2 to 6.7 keV. The y-axis shows the data-to-model ratio from 0 to 10. In the bottom panels, the x-axis shows the energy from 6.2 to 6.7 keV. The y-axis shows the data-to-model ratio from 0 to 5.

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