Area of research
Astronomy and Astrophysics · Spectroscopy
Research interest
Research focused on Astrophysics and Millimeter, with related work in Star formation, Aerosol, Protein filament. Notable publications include 'ATOMS: ALMA Three-millimeter Observations of Massive Star-forming regions – I. Survey description and a first look at G9.62+0.19', 'The Brick’ is not a brick : a comprehensive study of the structure and dynamics of the central molecular zone cloud G0.253+0.016', and 'FRAGMENTATION OF MASSIVE DENSE CORES DOWN TO ≲ 1000 AU: RELATION BETWEEN FRAGMENTATION AND DENSITY STRUCTURE'.
Gravitationally bound gas determines star formation in the Galaxy
Magnetic field morphology and evolution in the Central Molecular Zone and its effect on gas dynamics
CMZoom. IV. Incipient High-mass Star Formation throughout the Central Molecular Zone
ATOMS: ALMA Three-millimeter Observations of Massive Star-forming regions – XV. Steady accretion from global collapse to core feeding in massive hub-filament system SDC335
ATOMS: ALMA Three-millimeter Observations of Massive Star-forming regions – XI. From inflow to infall in hub-filament systems
ATOMS: ALMA Three-millimeter Observations of Massive Star-forming regions – VIII. A search for hot cores by using C2H5CN, CH3OCHO, and CH3OH lines
ATOMS: ALMA three-millimeter observations of massive star-forming regions – III. Catalogues of candidate hot molecular cores and hyper/ultra compact H <scp>ii</scp> regions
Calibrating the Davis–Chandrasekhar–Fermi Method with Numerical Simulations: Uncertainties in Estimating the Magnetic Field Strength from Statistics of Field Orientations
Star formation in ‘the Brick’: ALMA reveals an active protocluster in the Galactic centre cloud G0.253+0.016
ATOMS: ALMA Three-millimeter Observations of Massive Star-forming regions – I. Survey description and a first look at G9.62+0.19
CMZoom: Survey Overview and First Data Release
CMZoom. II. Catalog of Compact Submillimeter Dust Continuum Sources in the Milky Way’s Central Molecular Zone
‘The Brick’ is not a<i>brick</i>: a comprehensive study of the structure and dynamics of the central molecular zone cloud G0.253+0.016
Massive and low-mass protostars in massive "starless'' cores
Star formation in a high-pressure environment: an SMA view of the Galactic Centre dust ridge
Estimating ground-level PM <sub>2.5</sub> in eastern China using aerosol optical depth determined from the GOCI satellite instrument
FRAGMENTATION OF MASSIVE DENSE CORES DOWN TO ≲ 1000 AU: RELATION BETWEEN FRAGMENTATION AND DENSITY STRUCTURE