Search

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation
Large resolution
Hi-Resolution Export to PDF

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 5.

Distributions of the Stokes parameters I (left), Q (middle), and U (right) for synthetic dust polarization. We consider two distinct frequencies: 353 GHz (top), corresponding to Planck observations, and 150 GHz (bottom), a primary target for future CMB experiments.

Other Images in This Article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Copyright and Terms & Conditions

Additional terms of reuse