Properties of the cosmological filament between two clusters: A possible detection of a large-scale accretion shock by Suzaku H. Akamatsu, Y. Fujita, T. Akahori, Y. Ishisaki, K. Hayashida, A. Hoshino, F. Mernier, K. Yoshikawa, K. Sato and J. S. KaastraA&A, 606 (2017) A1DOI: https://doi.org/10.1051/0004-6361/201730497
