activity
20192026
most citedDust polarized emission observations of NGC 6334; BISTRO reveals the details of the complex but organized magnetic field structure of the high-mass star-forming hub-filament network

84 citations · 590 across the 49 of their papers we have counts for

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Showing 2022Show all

10 papers · 1 filter

astro-ph.GA2022★ 24 cited

JCMT BISTRO Observations: Magnetic Field Morphology of Bubbles Associated with NGC 6334

Mehrnoosh Tahani, Pierre Bastien, Ray S. Furuya +142

We study the HII regions associated with the NGC 6334 molecular cloud observed in the sub-millimeter and taken as part of the B-fields In STar-forming Region Observations (BISTRO)…

astro-ph.GA2022★ 26 cited

The JCMT BISTRO-2 Survey: Magnetic Fields of the Massive DR21 Filament

Tao-Chung Ching, Keping Qiu, Di Li +154

We present 850 m dust polarization observations of the massive DR21 filament from the B-fields In STar-forming Region Observations (BISTRO) survey, using the POL-2 polarimeter a…

astro-ph.GA2022★ 31 cited

The JCMT BISTRO Survey: A Spiral Magnetic Field in a Hub-filament Structure, Monoceros R2

Jihye Hwang, Jongsoo Kim, Kate Pattle +157

We present and analyze observations of polarized dust emission at 850 m towards the central 1 pc 1 pc hub-filament structure of Monoceros R2 (Mon R2). The data are obta…

astro-ph.GA2022★ 23 cited

Physical Modeling of Dust Polarization from Magnetically Enhanced Radiative Torque (MRAT) Alignment in Protostellar Cores with POLARIS

Nguyen Chau Giang, Thiem Hoang, Jeong-Gyu Kim +1

Magnetic fields () are an important factor that controls the star formation process. The leading method to observe is using polarized thermal emission from…

astro-ph.GA2022★ 12 cited

The JCMT BISTRO Survey: Multi-wavelength polarimetry of bright regions in NGC 2071 in the far-infrared/submillimetre range, with POL-2 and HAWC+

L. Fanciullo, F. Kemper, K. Pattle +31

Polarized dust emission is a key tracer in the study of interstellar medium and of star formation. The observed polarization, however, is a product of magnetic field structure, dus…

astro-ph.GA2022

Recent progress in theory and observational study of dust grain alignment and rotational disruption in star-forming regions

Le Ngoc Tram, Thiem Hoang

Modern understanding of dust astrophysics reveals that RAdiative Torques (RATs) arising from the radiation-dust interaction can induce two fundamental effects, including grain alig…

astro-ph.GA2022★ 23 cited

SOFIA observations of 30 Doradus: II -- Magnetic fields and large scale gas kinematics

Le Ngoc Tram, Lars Bonne, Yue Hu +13

The heart of the Large Magellanic Cloud, 30 Doradus, is a complex region with a clear core-halo structure. Feedback from the stellar cluster R136 has been shown to be the main…

astro-ph.GA2022★ 44 cited

On Internal and External Alignment of Dust Grains in Protostellar Environments

Thiem Hoang, Le Ngoc Tram, Vo Hong Minh Phan +3

We study the physical processes inducing the alignment of the grain axis of maximum inertia moment with the angular momentum (, i.e., internal alignment) and of …

astro-ph.GA2022★ 11 cited

Polarization, Polarizing Efficiency, and Grain alignment towards the direction of the cluster NGC 2345

Sadhana Singh, Jeewan C. Pandey, Thiem Hoang

We have investigated the grain alignment and dust properties towards the direction of the cluster NGC 2345 using the multi-band optical polarimetric observations. For the majority…

astro-ph.GA2022★ 41 cited

B-fields in Star-Forming Region Observations (BISTRO): Magnetic Fields in the Filamentary Structures of Serpens Main

Woojin Kwon, Kate Pattle, Sarah Sadavoy +149

We present 850 m polarimetric observations toward the Serpens Main molecular cloud obtained using the POL-2 polarimeter on the James Clerk Maxwell Telescope (JCMT) as part of th…