Nguyen Thi Thao

Morphology and kinematics of the gas envelope of protostar L1527 as obtained from ALMA observations of the C18O(2–1) line emission

Using ALMA observations of the C

12CO emission from the Red Rectangle

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Space reconstruction of the morphology and kinematics of axisymmetric radio sources

O(2-1) line emission of the gas envelope of protostar L1527, we have reconstructed its morphology and kinematics under the assumption of axisymmetry about the west-east axis. The main original contribution to our understanding of the formation process of L1527 is the presentation of a simple 3D parameterisation based solely on regions that are not dominated by absorption. In the explored range (

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

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The Vatly Radio Telescope: Performance Study

0.7 to 5 arcsec from the star) the model reproduces observations better than earlier attempts. The main results include: a measurement of the rotation velocity that confirms its evolution to Keplerian toward short distances; a measurement of the mean in-fall velocity, 0.43

Mapping Atomic Hydrogen in the Disk of the Milky Way

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Morphology of the

0.10 kms

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

, lower than free fall velocity, with no evidence for the significant

High-resolution ALMA observation of the 12CO(3–2) and 350 GHz continuum emissions of the debris disc of 49 Ceti

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