activity
20192022
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 · 215 across the 7 of their papers we have counts for

collaborators

8 papers

astro-ph.GA202212 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.GA202211 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.GA202241 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…

astro-ph.GA202084 cited

Dust 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

D. Arzoumanian, R. Furuya, T. Hasegawa +145

[Abridged] Filaments and hubs have received special attention recently thanks to studies showing their role in star formation. While the column density and velocity structures of b…

astro-ph.GA202022 cited

Modelling the strongest silicate emission features of local type 1 AGN

M. Martínez-Paredes, O. González-Martín, D. Esparza-Arredondo +8

We measure the 10 and m silicate features in a sample of 67 local () type 1 active galactic nuclei (AGN) with available {\it Spitzer} spectra dominated by non-stellar p…