Magnetic fields on different spatial scales of the L328 cloud
Shivani Gupta, Archana Soam, Janik Karoly, Chang Won Lee, Maheswar G

TL;DR
This study maps magnetic fields across multiple spatial scales in the L328 cloud, revealing their ordered structure and increasing strength towards smaller scales, with implications for core stability and star formation.
Contribution
It provides the first detailed core-scale magnetic field map of L328 using JCMT/POL-2, connecting large-scale and small-scale magnetic geometries.
Findings
Core-scale B-field strength is ~50.5 μG, 2.5 times higher than envelope.
Magnetic field is ordered and well-connected across scales.
The core is magnetically transcritical with a mass-to-flux ratio of 1.1.
Abstract
L328 core has three sub-cores S1, S2, and S3, among which the sub-core S2 contains L328-IRS, a Very Low Luminosity Object (VeLLO), which shows a CO bipolar outflow. Earlier investigations of L328 mapped cloud/envelope (parsec-scale) magnetic fields (B-fields). In this work, we used JCMT/POL-2 submillimeter (sub-mm) polarisation measurements at 850 m to map core-scale B-fields in L328. The B-fields were found to be ordered and well-connected from cloud to core-scales, i.e., from parsec- to sub-parsec-scale. The connection in B-field geometry is shown using dust polarisation maps to trace large-scale B-fields, optical and near-infrared (NIR) polarisation observations to trace B-fields in the cloud and envelope, and 850 m polarisation mapping core-scale field geometry. The core-scale B-field strength, estimated using the modified Davis-Chandrasekhar-Fermi relation, was…
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Ionosphere and magnetosphere dynamics · Astrophysics and Cosmic Phenomena
