activity
20242026
collaborators

16 papers

astro-ph.GA2026

Magneto-Gravitational Regulated Streamer Accretion onto a Class 0 Protostellar System

Bo Huang, Josep M. Girart, Ian W. Stephens +17

How do magnetic fields shape the way young stars gather gas from their birth clouds? Using high-resolution Atacama Large Millimeter/submillimeter Array observations of a young trip…

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

Magnetic field alignment with dense cores in the transition between cloud and core scales

Sean Yin, Ayush Pandhi, Rachel Friesen +7

In a magnetically-dominated model of star formation, we expect to see alignments between the magnetic field orientation of star-forming dense cores and the cloud-scale magnetic fie…

astro-ph.SR2026

Protostellar Outflows Shed Light on the Dominant Close Companion Star Formation Pathways

Ryan Sponzilli, Leslie Looney, John J. Tobin +11

Understanding the formation pathway for close-companion protostars is central to unraveling the processes that govern stellar multiplicity and very early star formation. We analyze…

astro-ph.GA2025

FIELDMAPS Data Release: Far-Infrared Polarization in the "Bones" of the Milky Way

Simon Coudé, Ian W. Stephens, Philip C. Myers +13

Polarization observations of the Milky Way and many other spiral galaxies have found a close correspondence between the orientation of spiral arms and magnetic field lines on scale…

astro-ph.GA2025

Magnetic Fields in the Bones of the Milky Way

Ian W. Stephens, Simon Coude, Philip C. Myers +20

Stars primarily form in galactic spiral arms within dense, filamentary molecular clouds. The largest and most elongated of these molecular clouds are referred to as ``bones," which…