Ding Luo

Massive stars at low metallicity

Stellar and wind properties of massive stars in the central parsec of the Galaxy

The non-LTE line formation of neutral carbon in late-type stars

A new extensive library of PHOENIX stellar atmospheres and synthetic spectra

Electron impact excitation collision strength for transitions in C II

The solar photospheric abundance of carbon

A Tale of Two Stars: The Extreme O7 Iaf+ Supergiant AV 83 and the OC7.5 III((f)) star AV 69

A super-Earth transiting a nearby low-mass star

parsec: stellar tracks and isochrones with the PAdova and TRieste Stellar Evolution Code

The solar photospheric abundance of carbon.Analysis of atomic carbon lines with the CO5BOLD solar model

CLOUDY 90: Numerical Simulation of Plasmas and Their Spectra

Massive stars at low metallicity: Evolution and surface abundances of O dwarfs in the SMC

A Grid of Non‐LTE Line‐blanketed Model Atmospheres of O‐Type Stars

Electron-impact excitation of Mg II: collision strengths and rate coefficients

SHINING, A Survey of Far-infrared Lines in Nearby Galaxies. I. Survey Description, Observational Trends, and Line Diagnostics

ATMOSPHERIC ESCAPE FROM HOT JUPITERS

MESA ISOCHRONES AND STELLAR TRACKS (MIST). I. SOLAR-SCALED MODELS

The Chemical Composition of the Sun

Atomic data for opacity calculations. XI. The carbon isoelectronic sequence

R-matrix calculations for electron-impact excitation ofC+,N2+, andO3+including fine structure

X-rays from colliding stellar winds

Atomic data for opacity calculations. X. Oscillator strengths and photoionisation cross sections for O III