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Ye Xu
Researcher at Beihang University
Publications - 385
Citations - 19429
Ye Xu is an academic researcher from Beihang University. The author has contributed to research in topics: Molecular cloud & Catalysis. The author has an hindex of 62, co-authored 364 publications receiving 16859 citations. Previous affiliations of Ye Xu include Louisiana State University & Rhodia.
Papers
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Journal ArticleDOI
Deposition of diamond-like carbon films on interior surface of long and slender quartz glass tube by enhanced glow discharge plasma immersion ion implantation
Ye Xu,Lidong Li,Paul K. Chu +2 more
TL;DR: In this article, a diamond-like carbon (DLC) films are deposited on the interior surface of 100mm long quartz glass tubes with inner diameters of 6, 4, and 0.9mm by enhanced glow discharge plasma immersion ion implantation (EGD-PIII) at 10kV.
Journal ArticleDOI
Local Molecular Gas toward the Aquila Rift Region
Yang Su,Ji Yang,Ji Yang,Qing-Zeng Yan,Yan Gong,Yan Gong,Zhiwei Chen,Shaobo Zhang,Yan Sun,Miaomiao Zhang,Xuepeng Chen,Xuepeng Chen,Xin Zhou,Min Wang,Hongchi Wang,Hongchi Wang,Ye Xu,Zhibo Jiang +17 more
TL;DR: In this article, the authors present the results of a ~250 square degrees CO mapping (+26d 4.1x10^5 ) in the whole region and show that the mass of the molecular gas is dominated by the W40 giant molecular cloud (GMC) at ~474pc (~1.4x10.5 ) and the GMC complex G036.0+01.0 at ~560-670pc (~2.0x10+1.5 ).
Journal ArticleDOI
Nonalcoholic fatty liver disease is associated with low-grade albuminuria in Chinese adults (change not displayed)
Lin Lin,Junxi Lu,Xiaolin Huang,Lin Ding,Yun Huang,Po Wang,Kui Peng,Dabing Zhang,Ye Xu,Min Xu,Yuhong Chen,Yu Fang Bi,Wei Qing Wang +12 more
TL;DR: NAFLD was significantly associated with an increased risk of present low-grade albuminuria in middle-aged and elderly Chinese men.
Journal ArticleDOI
Molecular gas toward the Gemini OB1 Giant Molecular Cloud Complex I: Observation data
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), the Lynds Dark Clouds and the West Front Clouds, the Swallow and Horn, and the Remote Clouds.