Image Details
Caption: Figure 4.
The distribution of f ICM in clumps identified in a snapshot of the tail of a simulated RPS galaxy (440 Myr in HDLV from Tonnesen & Bryan 2021) as a function of the distance from the galaxy. Gray dots refer to the values of clumps, while white hexagons indicate the median value at each given distance.
© 2021. The Author(s). Published by the American Astronomical Society.