葛继兴
研究员主要研究领域、方向
恒星形成区的天体化学模拟和射电观测研究。
代表性科研成果
1.Ge J, Mardones D, Inostroza-Pino N, et al. A three-dimensional chemical simulation with irregular density distributions of L1544. 2023, MNRAS, 521(2): 2833-2844.
2.Liu M, He J, Ge J, et al. Disk Dissipation, Giant Planet Formation, and Star Formation Rate Fluctuations in the 3 Myr History of Gould’s Belt. 2023,APJ, 943(1): 39.
3.Ge J. GGCHEMPY: A pure Python-based gas-grain chemical code for efficient simulation of interstellar chemistry. 2022, RAA, 22(1): 015004.
4.Ge J X, Mardones D, He J H, et al. Three-dimensional Projection Effects on Chemistry in a Planck Galactic Cold Clump.2020, APJ, 891(1): 36.
5.Ge J, Mardones D, Inostroza N, et al. The roles of polycyclic aromatic hydrocarbons in dark cloud chemistry: new constraints on sulphur-bearing species. 2020, MNRAS,497(3): 3306-3322.
6.Tang M, Ge J X, Qin S L, et al. Chemical Properties of Two Dense Cores in a Planck Galactic Cold Clump G168. 72-15.48. 2019, APJ, 887(2): 243.
7.Ge J X, He J H, Yan H R. Effects of turbulent dust grain motion to interstellar chemistry. 2016, MNRAS,455(4): 3570-3587.
8.Ge J X, He J H, Li A. Interstellar chemical differentiation across grain sizes.2016, MNRASL, 460(1): L50-L54.
9.Ge J X, He J H, Chen X, et al. Early-stage star-forming cloud cores in Galactic Legacy Infrared Mid-Plane Survey (GLIMPSE) extended green objects (EGOs) as traced by organic species. 2014,MNRAS, 445(2): 1170-1185.