Image Details
Caption: Figure 5.
The temperature distribution of gas particles in different types of structures for the GW (left panel), CM (middle panel), and LD (right panel) simulations. Black lines are for all gas particles and dark-red lines for all diffuse particles. The other color-coded lines are for gas particles in different components of the cosmic web as indicated. See the text for details of the analysis.
© 2022. The Author(s). Published by the American Astronomical Society.