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HomeNatureThe bulk motion of gas in the core of the Centaurus galaxy...

The bulk motion of gas in the core of the Centaurus galaxy cluster

  • As the leader of the Centaurus cluster target team in the XRISM Science Team, Y. Fujita led this research project and wrote the paper. K.S. is the sub-leader of the target team, led the data analysis and prepared the manuscript. He also contributed to the Resolve hardware development, integration tests, launch campaign, in-orbit operation and calibration. K.F., F.M., K. Matsushita, A. Simionescu, M.K. and A.M. analysed the data. Y. Fujita, K.S., K.F., F.M., K.M., A. Simionescu, and K. Nakazawa discussed the results. T.H., T.O., K.T., Y. M., M. Lowenstein, T. Yaqoob, E.D.M., M. Markevitch, F.S.P., M. Leutenegger, C.K. and R.K. contributed to the comments on data calibration and systematic errors, as well as on the content of the paper. M. Sun, K. Hosogi, N.W. and T.P. provided additional data and analysis. R.M., I.Z. and E.B. helped to improve the manuscript. The science goals of XRISM were discussed and developed over 7 years by the XRISM Science Team, all members of which are authors of this paper. All the instruments were prepared by the joint efforts of the team. The manuscript was subject to an internal collaboration-wide review process. All authors reviewed and approved the final version of the paper.

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