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A Cool Core Disturbed: Observational Evidence for the Coexistence of Subsonic Sloshing Gas and Stripped Shock-heated Gas around the Core of RX J1347.5–1145

  • Authors: Shutaro Ueda, Tetsu Kitayama, Masamune Oguri, Eiichiro Komatsu, Takuya Akahori, Daisuke Iono, Takumi Izumi, Ryohei Kawabe, Kotaro Kohno, Hiroshi Matsuo, Naomi Ota, Yasushi Suto, Shigehisa Takakuwa, Motokazu Takizawa, Takahiro Tsutsumi, and Kohji Yoshikawa

2018 The Astrophysical Journal 866 48.

  • Provider: AAS Journals

Caption: Figure 7.

Temperature of the excess component in units of keV (left) and its statistical error (right) inferred from the ALMA SZE and Chandra X-ray images, assuming a constant line-of-sight length of Lexcess = 150 kpc. The values are approximately proportional to ﹩{({L}_{\mathrm{excess}}/150\mathrm{kpc})}^{-1/2}﹩. Regions for which the S/Ns of either data sets are less than 4σ are left blank (black). For reference, the elliptical annuli shown in Figure 3 are overlaid. Note that X-ray spectra are not used in computing the quantities plotted in this figure.

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