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Evolution of Supernova Remnants in a Cloudy Multiphase Interstellar Medium

  • Authors: Minghao Guo, 明浩 郭, Chang-Goo Kim, James M. Stone

Minghao Guo et al 2025 The Astrophysical Journal 990 .

  • Provider: AAS Journals

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.

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