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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 2.

Residual images of the X-ray and SZE surface brightness. Left: the residual image of Chandra X-ray surface brightness after subtracting the mean profile, excluding the southeast quadrant. The original surface brightness is the same as in the left panel of Figure 1. For reference, the position of the central AGN is marked by a cross. Right: same as the left panel but for the ALMA 92 GHz brightness in mJy beam−1 with the effective beam size of 5″ FWHM. The original surface brightness is shown in the right panel of Figure 1.

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