Ye Xu

TL;DR: In this paper, a large-scale (CO)-C-12 (J = 1 -> 0) outflow survey was conducted toward the W3/4/5 complex and its surroundings.

TL;DR: In this paper, the authors present a study of the three-dimensional structure of the molecular clouds in the Galactic Centre (GC) using CO emission and OH absorption lines, and they find that the total mass of OH in the GC is in the range 2400-5100 solar mass.

TL;DR: In this article, a large-scale mapping toward the GEM OB1 association in the galactic anti-center direction is presented, which is divided into four main components based on spatial distribution and velocity: the Gemini OB1 Giant Molecular Cloud (GGMC) Complex, the Lynds Dark Clouds and the West Front Clouds, the Swallow and Horn, and the Remote Clouds.

TL;DR: In this paper, the authors conducted resonant angle-resolved photoemission spectroscopy of well-defined $c-CeO2$(111)-model surfaces, revealing distinct $f$ contributions in the valence band of the two compounds.

TL;DR: In this paper, the impact of the ionized radiation from the M 16 H II region on the surrounding molecular cloud and on its hosted star formation was investigated using new CO data and existing infrared, optical, and submillimeter data.