activity
20152026
most citedStudying magnetic fields and dust in M17 using polarized thermal dust emission observed by SOFIA/HAWC+

24 citations · 67 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.SR2026

A multiwavelength ALMA view of gas and dust in binary protoplanetary system AS 205: Evidence of dust asymmetric distribution

Nguyen Thi Phuong, Nguyen Tat Thang

We present Atacama Large Millimeter/Submillimeter Array observations of multi-wavelength dust emissions at 3.1 and 1.3 mm; along with molecular line emissions of CO(2-1), CO(3-2),…

astro-ph.SR2024

Early Planet Formation in Embedded Disks (eDisk) XIII: Aligned Disks with Non-Settled Dust Around the Newly Resolved Class 0 Protobinary R CrA IRAS 32

Frankie J. Encalada, Leslie W. Looney, Shigehisa Takakuwa +19

Young protostellar binary systems, with expected ages less than 10 years, are little modified since birth, providing key clues to binary formation and evolution. We prese…

astro-ph.SR2024★ 8 cited

Evidence of Grain Alignment by Magnetically Enhanced Radiative Torques from Multiwavelength Dust Polarization Modeling of HL Tau

Nguyen Tat Thang, Pham Ngoc Diep, Thiem Hoang +4

Atacama Large Millimeter/Submillimeter Array (ALMA) has revolutionized the field of dust polarization in protoplanetary disks across multiple wavelengths. Previous observations and…

astro-ph.GA2023★ 21 cited

B-fields And dust in interstelLar fiLAments using Dust POLarization (BALLAD-POL): I. The massive filament G11.11-0.12 observed by SOFIA/HAWC+

Nguyen Bich Ngoc, Pham Ngoc Diep, Thiem Hoang +8

We report the first measurement of polarized thermal dust emission toward the entire early and massive Infrared Dark Cloud G11.110.12 taken by the polarimeter SOFIA/HAWC+ at 214…

astro-ph.GA2021★ 3 cited

On planet formation around supermassive black holes and the grain disruption barriers by radiative torques

Nguyen Chau Giang, Thiem Hoang, Le Ngoc Tram +5

It has recently been suggested that planets can form by dust coagulation in the torus of active galactic nuclei (AGN) with low luminosity of $L_{\rm bol}\lesssim 10^{42} erg s^{-1}…

astro-ph.GA2021★ 3 cited

Modeling extinction and reddening effects by circumstellar dust in the Betelgeuse envelope in the presence of radiative torque disruption

Bao Truong, Le Ngoc Tram, Thiem Hoang +9

Circumstellar dust is formed and evolved within the envelope of evolved stars, including Asymptotic Giant Branch (AGB) and Red Supergiant (RSG). The extinction of stellar light by…

astro-ph.GA2021★ 24 cited

Studying magnetic fields and dust in M17 using polarized thermal dust emission observed by SOFIA/HAWC+

Thuong Duc Hoang, Nguyen Bich Ngoc, Pham Ngoc Diep +12

We report the highest spatial resolution measurement of magnetic fields in M17 using thermal dust polarization taken by SOFIA/HAWC+ centered at 154 m wavelength. Using the Davis…

astro-ph.SR2018★ 1 cited

Morphology of the CO(3-2) millimeter emission across the gas disc surrounding the triple protostar GG Tau A using ALMA observations

N. T. Phuong, P. N. Diep, A. Dutrey +8

Observations by the Atacama Large Millimeter/sub-millimeter Array of the dust continuum and CO(3-2) millimeter emissions of the triple stellar system GG Tau A are analysed,…

astro-ph.SR2016★ 2 cited

Morphology and kinematics of the gas envelope of the Mira binary W Aquilae

D. T. Hoai, P. T. Nhung, P. N. Diep +4

We analyse ALMA observations of the 12CO(3-2) emission of the circumstellar envelope (CSE) of the Mira variable binary star W Aql. These provide, for the first time, spatially reso…

astro-ph.SR2016★ 1 cited

Morphology and kinematics of the gas envelope of the variable AGB star Gruis

P. T. Nhung, D. T. Hoai, P. N. Diep +4

Observations of the CO(3-2) emission of the circumstellar envelope (CSE) of the variable star Gru using the compact array (ACA) of the ALMA observatory have been recen…

astro-ph.SR2015★ 4 cited

CO emission from the Red Rectangle

Pham Tuan Anh, Pham Ngoc Diep, Do Thi Hoai +4

Observations of an unprecedented quality made by ALMA on the Red Rectangle of CO(3-2) and CO(6-5) emissions are analysed jointly with the aim of obtaining as simple as possible a d…