Image Details
Caption: Figure 7.
T − n joint distribution for all gas (first column), gas that is initially CNM (species C 0; second column) and WNM (species C 2 ; third column), and T − v joint distribution (last column) of the gas at 10 kyr (t/t sf,WNM ≈ 0.3, t/t sf,CNM ≈ 4) without (upper panel) and with (lower panel) thermal conduction. Annotated are the main components of the ISM, along with a significant fraction occupying intermediate regions. Dashed lines in the last column mark the boundary of ∣v∣ = 5 km s−1 and T = 5050 K used for the definition of gas phases to distinguish the three components. Thermal conduction increases the contribution of CNM to hot gas.
© 2025. The Author(s). Published by the American Astronomical Society.