王科
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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. Currently, he mainly works on three projects:(1) resolving starless infrared dark clouds; he has discovered one of the few known high-mass prestellar cores, a long-sought key observable for a leading theoretical model of star formation;(2) a Galaxy-wide census of the largest molecular filaments; he has made the first census of the densest, coldest, velocity-coherent large-scale (>10 pc) filaments in the Milky Way; and(3) a systematic survey of dense molecular clouds in the outer Galaxy; he is principal investigator of the ESO Public Survey SAMPLING (SMT \研究领域
Star formation, interstellar medium, radio interferometry近期论文
ESA Feature Article: Herschel's hunt for filaments in the Milky WayAAS NOVA Feature: Building Up the Milky Way’s SkeletonHarvard CfA Press Release: SMA Unveils How Small Cosmic Seeds Grow Into Big Stars标签:
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- 王科 05-06
- 王然 05-06
- 吴学兵 05-06
- 邵立晶 05-06
- Richard de Grijs 05-06
- Rainer Spurzem 05-06
- 彭逸西 05-06
- 彭影杰 05-06
- Pau Amaro-Seoane 05-06
- Martin C. Smith 05-06