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Image credits: ESA & Planck Collaboration
project a1: investigating the influence of magnetic fields and local conditions (radiation & gas) on Dust Alignment, Dust Evolution (Growth and Disruption), and dust extinction/emission/polarization
project a1: investigating the influence of magnetic fields and local conditions (radiation & gas) on Dust Alignment, Dust Evolution (Growth and Disruption), and dust extinction/emission/polarization
Image credits: Thiem Hoang, KASI
Project A2: SYN-POL: Synthetic dust Polarization Observations by post-processing Multi-scale MHD Simulations of Star Formation, from the ISM, Molecular clouds, & Filaments to protostellar cores
Project A2: SYN-POL: Synthetic dust Polarization Observations by post-processing Multi-scale MHD Simulations of Star Formation, from the ISM, Molecular clouds, & Filaments to protostellar cores
Project A3: BALLAD-POL: probing magnetic fields (B-fields) and Dust Physics in Interstellar Filaments using starlight and thermal Dust Polarization
Project A3: BALLAD-POL: probing magnetic fields (B-fields) and Dust Physics in Interstellar Filaments using starlight and thermal Dust Polarization
Project A4: 3D BISTRO: Probing 3D magnetic fields in the ISM and Star-Forming Regions using dust Polarization (starlight and thermal emission) and other techniques (Zeeman effect, Synchrotron, and Gradient Techniques)
Project A4: 3D BISTRO: Probing 3D magnetic fields in the ISM and Star-Forming Regions using dust Polarization (starlight and thermal emission) and other techniques (Zeeman effect, Synchrotron, and Gradient Techniques)
From Truong & Hoang (2025, ApJ)
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