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Galactic Dust Polarization in Turbulent Multiphase ISM: On the Origin of the EE/BB Asymmetry

  • Authors: Yue Hu, Bao Truong, Thiem Hoang, Le Ngoc Tram

Yue Hu et al 2026 The Astrophysical Journal 1007 .

  • Provider: AAS Journals

Caption: Figure 1.

Distributions of number density n, temperature T, and turbulent plasma beta βtur in the multiphase ISM simulation. Shown is a two-dimensional slice from the 20483 simulation, displaying the number density (top), temperature (middle), and turbulent plasma beta βtur = ρv2/(B2/8π) (bottom), where ρ is the gas mass density and v is the local turbulent velocity. For visualization purposes, only half of each slice is shown. The CNM, characterized by low temperature, is spatially correlated with the densest regions.

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