葛宏伟，男，中国科学院云南天文台研究员。2010年7月获中国科学院云南天文台博士学位，并入职中国科学院云南天文台工作至今。2013.01-2014.01和2018.05-2019.05美国伊利诺伊大学访问学者；2022.01-2023.01英国剑桥大学访问学者。本人长期从事恒星物理、双星演化相关领域，特别是双星快速物质交换研究。针对双星物质交换过程，我们建立了恒星的绝热和热平衡物质损失模型；相关成果被国际同行评价为：“可以形成一本教科书”、被国家基金委遴选为“聚焦前沿、独辟蹊径”典型案例。截至2023年10月共发表SCI论文17篇，被引1242次（谷歌学术）。

[1] Hongwei Ge, Christopher A Tout, Xuefei Chen, Arnab Sarkar, Dominic J Walton, Zhanwen Han. Criteria for Dynamical Timescale Mass Transfer of Metal-poor Intermediate-mass Stars. THE ASTROPHYSICAL JOURNAL[J]. 2023, 945(1), id 7;

[2] Ge, Hongwei, Webbink, Ronald F, Chen, Xuefei, Han, Zhanwen. Adiabatic Mass Loss in Binary Stars. III. From the Base of the Red Giant Branch to the Tip of the Asymptotic Giant Branch. ASTROPHYSICAL JOURNAL[J]. 2020, 899(2), id 132;

[3] Ge, Hongwei, Webbink, Ronald F, Han, Zhanwen. The Thermal Equilibrium Mass-loss Model and Its Applications in Binary Evolution. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES[J]. 2020, 249(1), id 9;

[4] Han, ZhanWen, Ge, HongWei, Chen, XueFei, Chen, HaiLiang. Binary Population Synthesis. RESEARCH IN ASTRONOMY AND ASTROPHYSICS[J]. 2020, 20(10): 207-220;

[5] Ge, Hongwei, Webbink, Ronald F, Chen, Xuefei, Han, Zhanwen. ADIABATIC MASS LOSS IN BINARY STARS. II. FROM ZERO-AGE MAIN SEQUENCE TO THE BASE OF THE GIANT BRANCH. ASTROPHYSICAL JOURNAL[J]. 2015, 812(1), id 40;

[6] Ivanova, N, Justham, S, Chen, X, De Marco, O, Fryer, C L, Gaburov, E, Ge, H, Glebbeek, E, Han, Z, Li, X D, Lu, G, Marsh, T, Podsiadlowski, P, Potter, A, Soker, N, Taam, R, Tauris, T M, van den Heuvel, E P J, Webbink, R F. Common envelope evolution: where we stand and how we can move forward. ASTRONOMY AND ASTROPHYSICS REVIEW[J]. 2013, 21;

[7] Ge, Hongwei, Hjellming, Michael S, Webbink, Ronald F, Chen, Xuefei, Han, Zhanwen. ADIABATIC MASS LOSS IN BINARY STARS. I. COMPUTATIONAL METHOD. ASTROPHYSICAL JOURNAL[J]. 2010, 717(2): 724-738