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astro-ph.GA2025

TRAO Survey of the Nearby Filamentary Molecular Clouds, the Universal Nursery of Stars (TRAO-FUNS). IV. Filaments and Dense Cores in the W40 and Serpens South Regions of Aquila

Satyajeet Moharana, Chang Won Lee, Shinyoung Kim +9

We present the results of molecular line observations toward the W40 and Serpens South regions of the Aquila molecular cloud complex, conducted as part of the TRAO-FUNS project to…

astro-ph.GA2025

Unbound Tails and Compressed Heads: A JCMT Study of the SFO 38 Cloud

Puja Porel, Archana Soam, Janik Karoly +5

SFO 38, located in the Cepheus molecular cloud within the northern part of the HII region IC 1396, is shaped by intense ultraviolet radiation from the nearby O6.5V-type star HD 206…

astro-ph.GA2025

Investigating the Kinematics of Molecular Gas in Cometary Globule L1616

Puja Porel, Archana Soam, Janik Karoly +2

LDN 1616 is a cometary globule located approximately 8 degrees west of the Orion OB1 associations. The massive OB stars in the Orion belt region act as catalysts, triggering the st…

astro-ph.GA2025

B-fields And dust in interstelLar fiLAments using Dust POLarization (BALLAD-POL): IV. Grain alignment mechanisms in Cocoon Nebula (IC 5146) using polarization observations from JCMT/POL-2

Saikhom Pravash, Thiem Hoang, Archana Soam +4

The polarization of starlight and thermal dust emission from aligned non-spherical grains provides a powerful tool for tracing magnetic field morphologies and strengths in diffuse…

astro-ph.GA2025

The JCMT BISTRO-3 Survey: Variation of magnetic field orientations on parsec and sub-parsec scales in the massive star-forming region G28.34+0.06

Jihye Hwang, Kate Pattle, Chang Won Lee +35

Magnetic fields play a significant role in star-forming processes on core to clump scales. We investigate magnetic field orientations and strengths in the massive star-forming clum…

astro-ph.GA2025

The JCMT BISTRO Survey: Magnetic Fields Align with Orbital Structure in the Galactic Center

Janik Karoly, Derek Ward-Thompson, Kate Pattle +29

We present the magnetic field in the dense material of the Central Molecular Zone (CMZ) of the Milky Way, traced in 850 m polarized dust emission as part of the James Clerk Max…