Figure 9 from 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

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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 9.

Surface mass density map of RX J1347.5–1145 measured with SL assuming two (left) or three (right) dark halo components in units of 10¹⁵ h ﹩{M}_{\odot }﹩ Mpc⁻². The entire morphology is nearly unchanged by addition of the third dark matter component.

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