activity
20152020
most citedThe morpho-kinematics of the circumstellar envelope around the AGB star EP Aqr

18 citations · 44 across the 5 of their papers we have counts for

collaborators

7 papers

astro-ph.SR20208 cited

Revealing new features of the millimetre emission of the circumbinary envelope of Mira Ceti

D. T. Hoai, P. Tuan-Anh, P. T. Nhung +4

We study the morpho-kinematics of the circumbinary envelope of Mira Ceti between 100 and 350 au from the stars using ALMA observations of the SiO (=0, =5-4) and C…

astro-ph.SR2020

GG Tau A: gas properties and dynamics from the cavity to the outer disk

N. T. Phuong, A. Dutrey, P. N. Diep +13

We used new ALMA CO and CO(3-2) observations obtained at high angular resolution (0.2") together with previous CO(3-2) and (6-5) ALMA data and continuum maps at…

astro-ph.SR2019

The nascent wind of AGB star R Doradus: evidence for a recent episode of enhanced mass loss

P. T. Nhung, D. T. Hoai, P. Tuan-Anh +4

We analyse ALMA observations of the SO() emission of the circumstellar envelope of oxygen-rich AGB star R Dor, probing distances between 20 and 100 au from the star wh…

astro-ph.SR201916 cited

Observation of narrow polar jets in the nascent wind of oxygen-rich AGB star EP Aqr

P. Tuan-Anh, D. T. Hoai, P. T. Nhung +6

Using ALMA observations of CO(2-1), SiO(5-4) and SO(16-17) emissions of the circumstellar envelope of AGB star EP Aqr, we describe the mo…

astro-ph.SR20192 cited

The protoplanetary disc of HD 163296 as observed by ALMA

P. N. Diep, D. T. Hoai, N. B. Ngoc +4

HD 163296 is one of the few protoplanetary discs displaying rings in the dust component. The present work uses ALMA observations of the 0.9 mm continuum emission having significant…

astro-ph.SR201918 cited

The morpho-kinematics of the circumstellar envelope around the AGB star EP Aqr

D. T. Hoai, P. T. Nhung, P. Tuan-Anh +6

ALMA observations of CO(1-0) and CO(2-1) emissions of the circumstellar envelope of EP Aqr, an oxygen-rich AGB star, are reported. A thorough analysis of their properties is presen…