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The Hot Universe with XRISM and Athena

Published online by Cambridge University Press:  07 April 2020

M. Guainazzi  and
M. S. Tashiro
M. Guainazzi
Affiliation:
ESTEC/ESA, Keplerlaan 1, 2201AZ Noordwijk, The Netherlands email: Matteo.Guainazzi@sciops.esa.int
M. S. Tashiro
Affiliation:
ISAS/JAXA, 3-1-1 Yoshinodai, Chuo-ku, Sagamihara, Kanazgawa 252-5210, Japan email: tashiro@astro.isas.jaxa.jp Graduate School of Science and Engineering, Saitama University, 255 Shimo-Okubo, Sakawa, Saitama, Saitama 338-8570, Japan email: tashiro@phy.saitama-u.ac.jp
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Abstract

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X-ray spectroscopy is key to address the theme of “The Hot Universe”, the still poorly understood astrophysical processes driving the cosmological evolution of the baryonic hot gas traceable through its electromagnetic radiation. Two future X-ray observatories: the JAXA-led XRISM (due to launch in the early 2020s), and the ESA Cosmic Vision L-class mission Athena (early 2030s) will provide breakthroughs in our understanding of how and when large-scale hot gas structures formed in the Universe, and in tracking their evolution from the formation epoch to the present day.

Keywords

space vehicles: instrumentstelescopesX-rays: general
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 14 , Symposium S342: Perseus in Sicily: From Black Hole to Cluster Outskirts , May 2018 , pp. 29 - 36
Copyright
© International Astronomical Union 2020

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