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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 7.

Ratio of CEE to CBB from synthetic dust polarization at 353 GHz. Top panel: EE and BB power spectra computed from synthetic dust polarization maps with cold gas (T  <  200 K) excluded. The shaded area overlapping the line represents the standard deviation. The gray region denotes the range of CEE/CBB ratios measured by Planck. kinj is the injection wavenumber of turbulence, and kdis is the numerical dissipation wavenumber. Bottom panel: same as the top panel, but showing spectra computed separately from different gas phases: WNM (T  >  5000 K; red), UNM (200 K <T <  5000 K; green), and CNM (T  <  200 K; blue).

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