Stereological comparison of simulated projections to the eRASS1 ellipticity distribution yields most-probable axial ratios (1.51 ± 0.27, 1.17 ± 0.27) favoring prolate shapes.
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The three-dimensional shapes of the galaxy cluster intracluster medium in eRASS1
Stereological comparison of simulated projections to the eRASS1 ellipticity distribution yields most-probable axial ratios (1.51 ± 0.27, 1.17 ± 0.27) favoring prolate shapes.