activity
20242026
collaborators

16 papers

astro-ph.GA2026

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

Yue Hu, Bao Truong, Thiem Hoang +1

Polarized thermal emission from Galactic dust is the dominant foreground for CMB polarization measurements at high frequencies, with its statistical properties shaped by the interp…

astro-ph.GA2026

Probing Anomalous Microwave Emission with the Square Kilometre Array

Matías Vidal, Simón Casassus, Roke Cepeda-Arroita +15

Anomalous microwave emission (AME) represents an excess of radiation in the 10-60 GHz range, distinct from synchrotron, free-free, or thermal dust emission. Although most commonly…

astro-ph.GA2026

The magnetic field in the Milky Way Galaxy: from large to small scales

Xiaohui Sun, Jennifer West, Marijke Haverkorn +6

The Milky Way is the galaxy in which we can study its magnetic field to the finest details, providing an ideal laboratory to understand the fundamental questions: how magnetic fiel…

astro-ph.GA2026

3D B-fieLds in the InterStellar medium and Star-forming regions (3D-BLISS): I. Using Starlight Polarization in the Massive IRDC Filament G11.11-0.12

Bao Truong, Thiem Hoang, Nguyen Bich Ngoc +3

Measuring three-dimensional magnetic fields (3D B-fields) is essential to understand the formation and evolution of the interstellar medium and multi-scale star formation; however,…

astro-ph.GA2026

BISTRO Survey: Gravity-Dominated and Magnetically Regulated Star Formation in M17 SW

Mengke Zhao, Keping Qiu, Ji-hyun Kang +27

We present high-resolution magnetic field maps of the M17 SW molecular cloud using JCMT 850 m dust polarization at a scale of 14. The magnetic field exhibits a distinct arc…

astro-ph.GA2026

One-dimensional and time-dependent modelling of complex organic molecules in protostars

Le Ngoc Tram, Serena Viti, Katarzyna M. Dutkowska +5

Complex organic molecules (COMs), the building blocks of life, have been extensively detected under various physical conditions, from quiescent clouds to star-forming regions. They…