activity
20242026
collaborators
Showing astro-ph.GAShow all

11 papers · 1 filter

astro-ph.GA2026

Measuring Magnetic Fields Near and Far with the SKA via the Zeeman Effect

Timothy Robishaw, Marta Nowotka, Tao-Chung Ching +7

Zeeman splitting in spectral lines -- both in emission and absorption -- provides direct estimates of magnetic field strength and direction in magnetized gas in our own Milky Way a…

astro-ph.GA2026

Measuring Magnetic Field Strengths in Galactic Star-forming Regions via the Zeeman Effect with the SKA

Tyler L. Bourke, Tao-Chung Ching, Laura Fissel +14

Magnetic fields thread the interstellar medium from the largest to the smallest scales and play an important role in molecular cloud evolution and star formation. Quantifying this…

astro-ph.GA2026

Star Formation Drives Production of Low Energy Cosmic Rays

Ningyu Tang, Jiahao Liu, Di Li +18

For over a century, the origin of low-energy cosmic rays (LECRs), the dominant heaters and ionizers of dense interstellar gas, remains elusive owing to solar modulation and uncerta…

astro-ph.GA2026

ALMA Polarization Study of the Magnetic Fields in Two Massive Clumps in the 20 km s Cloud of the Central Molecular Zone

Yuhua Liu, Xing Lu, Junhao Liu +14

We present the Atacama Large Millimeter/submillimeter Array (ALMA) observations of linearly polarized 870 m continuum emission at a resolution of 0.2 (20…

astro-ph.GA2025

Pinched Magnetic Fields in the High-mass Protocluster W3 IRS5

Huei-Ru Vivien Chen, Qizhou Zhang, Tao-Chung Ching +2

We present polarization maps of dust emission at 340 GHz in the luminous high-mass protocluster, W3 IRS5, observed with the Submillimeter Array. The projected magnetic fields appea…

astro-ph.GA2025

Joint Analysis of HI Absorption Zeeman Measurements and the Morphology of Filamentary HI Emission

Marta Nowotka, Susan E. Clark, Blakesley Burkhart +4

We present a joint analysis of HI absorption Zeeman measurements and the morphology of filamentary HI emission to investigate the three-dimensional structure of the magnetic field…