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Locating the Warm-Hot Intergalactic Medium in the Simulated Local Universe

K. Yoshikawa·K. Dolag·Y. Suto·S. Sasaki·N. Y. Yamasaki·T. Ohashi·K. Mitsuda·Y. Tawara·R. Fujimoto·T. Furusho·A. Furuzawa·M. Ishida·Y. Ishisaki·Y. Takei
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Abstract

We present an analysis of mock spectral observation of warm-hot intergalactic medium (WHIM) using a constrained simulation of the local universe. The simulated map of oxygen emission lines from local WHIM reproduces well the observed structures traced by galaxies in the real local universe. We further attempt to perform mock observations of outer parts of simulated Coma cluster and A3627 adopting the expected performance of DIOS (Diffuse Intergalactic Oxygen Surveyor), which is proposed as a dedicated soft X-ray mission to search for cosmic missing baryons. We find that WHIMs surrounding nearby clusters are detectable with a typical exposure time of a day, and thus constitute realistic and promising targets for DIOS. We also find that an X-ray emitting clump in front of Coma cluster, recently reported in the XMM-Newton observation, has a counterpart in the simulated local universe, and its observed spectrum can be well reproduced in the simulated local universe if the gas temperature is set to the observationally estimated value.

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K. Yoshikawa, K. Dolag, Y. Suto, S. Sasaki, N. Y. Yamasaki, T. Ohashi, K. Mitsuda, Y. Tawara, R. Fujimoto, T. Furusho, A. Furuzawa, M. Ishida, Y. Ishisaki, Y. Takei. 2004-09-27. Locating the Warm-Hot Intergalactic Medium in the Simulated Local Universe. https://doi.org/10.1093/pasj%2F56.6.939

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