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Ke Wang observes high-mass star formation at high-resolution. He is an expert in submillimeter interferometry and has served in the European ALMA Regional Center and the SMA operations team for more than 5 years. His research characterizes the initial conditions of high-mass star formation throughout the Galaxy by observing various samples of molecular clouds in different Galactic environments. Observations at multiple scales are made using submm/mm/cm interferometers including ALMA, SMA, and VLA, and space- and ground-based single-dish telescopes including Herschel, GBT 100m, Effelsberg 100m, Nobeyama 45m, IRAM 30m, JCMT 15m, APEX 12m, CSO 10m, and SMT 10m.
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论文共 153 篇作者统计合作学者相似作者
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ASTROPHYSICAL JOURNAL SUPPLEMENT SERIESno. 1 (2024)
The Astrophysical Journal Supplement Seriesno. 1 (2024): 9
The Astrophysical Journal Lettersno. 1 (2024): L9
Chao Wang,Ke Wang,Feng-Wei Xu,Patricio Sanhueza,Hauyu Baobab Liu,Qizhou Zhang,Xing Lu, F. Fontani,Paola Caselli,Gemma Busquet,Jonathan C. Tan,Di Li,
ASTRONOMY & ASTROPHYSICS (2024)
Astronomy & Astrophysics (2024)
arxiv(2024)
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C. Zhang,Feng-Yao Zhu, Shipeng Li, Z. -Y. Ren, H. -L. Liu,Ke Wang, J. -W. Wu, Y. Zhang, J. -W. Zhou, K. Tatematsu,Guido Garay,Anandmayee Tej,
arXiv (Cornell University) (2023)
ASTROPHYSICAL JOURNALno. 1 (2023): 40-40
Behavioural brain research (2023): 114710
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