activity
20162021
most citedThe morpho-kinematics of the circumstellar envelope around the AGB star EP Aqr

18 citations · 56 across the 5 of their papers we have counts for

collaborators

15 papers

astro-ph.SR202114 cited

An unbiased NOEMA 2.6 to 4 mm survey of the GG Tau ring: First detection of CCS in a protoplanetary disk

N. T. Phuong, A. Dutrey, E. Chapillon +13

Molecular line surveys are among the main tools to probe the structure and physical conditions in protoplanetary disks (PPDs), the birthplace of planets. The large radial and verti…

astro-ph.GA2021

Morpho-kinematics of the molecular gas in a quasar host galaxy at redshift =0.654

T. T. Thai, P. Tuan-Anh, P. Darriulat +5

We present a new study of archival ALMA observations of the CO(2-1) line emission of the host galaxy of quasar RX J1131 at redshift =0.654, lensed by a foreground galaxy. A simp…

astro-ph.SR2021

Morpho-kinematics of the circumstellar envelope of the AGB star R Dor: a global view

P. T. Nhung, D. T. Hoai, P. Tuan-Anh +5

We analyse new ALMA observations of the SiO (=0, =87) and SO(=0, ) line emissions of the circumstellar envelope (CSE) of the oxygen-…

astro-ph.GA2020

Quadruply-imaged quasars: some general features

P. Tuan-Anh, T. T. Thai, N. A. Tuan +6

Gravitational lensing of point sources located inside the lens caustic is known to produce four images in a configuration closely related to the source position. We study this rela…

astro-ph.GA2020

CHIMPS2: Survey description and CO emission in the Galactic Centre

D. J. Eden, T. J. T. Moore, M. J. Currie +103

The latest generation of Galactic-plane surveys is enhancing our ability to study the effects of galactic environment upon the process of star formation. We present the first data…

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…