仝号教授
教育背景 博士
研究领域 天体物理
研究方向 脉冲星，磁星，中子星
电子邮箱 tonghao@gzhu.edu.cn
所在系所 天文系物理与材料科学学院
办公地点 行政西楼前座546
▍个人简介
2010年博士毕业于南京大学，中国科学院高能所博士后（2010-2012），中国科学院新疆台副研究员（2012-2017），2017年后入职广州大学。主讲本科生的《光学》，研究生的《辐射机制》《高能天体物理》等课程。主要从事脉冲星、磁星方向的理论研究，以第一作者或通讯作者发表SCI科研论文20余篇，总引用300多次。主持了国家自然科学基金的面上项目、青年基金和若干省部级项目。
▍担任主要课程
本科生课程：《光学》
研究生课程：《辐射机制》
▍主持课题
1. “孤立磁星和吸积磁星的磁层研究”，国家自然科学基金面上项目，2018-2021，主持
2. 中国科学院青年创新促进会会员项目，2013-2016，主持
3. “AXP/SGR多波段辐射特性研究”，国家自然科学基金青年项目，2012-2014，主持
▍主要论文
一、代表性论著
(1)Tong, H.*; Xu, R. X.; Song, L. M.; Qiao, G. J.; Wind braking of magnetars,Astrophysical Journal, 2013, 768(2): 144. (期刊论文)
(2) Kou, F. F.;Tong, H.*; Rotational evolution of the Crab pulsar in the wind braking model ,Monthly Notices of the Royal Astronomical Society, 2015, 450(2): 1990-1998. (期刊论文)
(3)Tong, H.*; Large polar caps for twisted magnetosphere of magnetars ,Monthly Notices of the Royal Astronomical Society, 2019, 489(3): 3769-3777. (期刊论文)
(4)Tong, H.*; Wang, W.; Liu, X. W.; Xu, R. X.; Rotational evolution of magnetars in the presence of a fallback disk,Astrophysical Journal, 2016, 833(2): 265. (期刊论文)
(5)Tong, H.*; Wang, W*; Accreting magnetars: linking ultraluminous X-ray pulsars and the slow pulsation X-ray pulsars ,Monthly Notices of the Royal Astronomical Society, 2019, 482(4): 4956-4964. (期刊论文)
二、已发表的其余论著（按时间倒序排序）
(1)Tong, H.*; Wang, P. F.; Wang, H. G.; Yan, Z.; Rotating vector model for magnetars,MNRAS, 2021, 502: 1549-1556. (期刊论文)
(2)Tong, H.*; Huang, L.; Magnetar outburst and spin-down glitch ,Monthly Notices of the Royal Astronomical Society, 2020, 497(3): 2680-2687. (期刊论文)
(3)Tong, Hao*; Wang, Wei; Wang, Hong-Guang; Periodicity in fast radio bursts due to forced precession by a fallback disk ,Research in Astronomy and Astrophysics, 2020, 20(9): 0-142. (期刊论文)
(4) Kou, F F;Tong, H.*; Xu, R X; Zhou, X; Rotational Evolution of the Slowest Radio Pulsar, PSR J0250 5854,Astrophysical Journal, 2019, 876(2): 131. (期刊论文)
(5)Tong, Hao*; Yu, Cong*; Huang, Lei; A magnetically driven origin for the low luminosity GRB 170817A associated with GW170817 ,Research in Astronomy and Astrophysics, 2018, 18(6): 0-67. (期刊论文)
(6)Tong, H.*; Kou, F F; Possible Evolution of the Pulsar Braking Index from Larger than Three to About One ,Astrophysical Journal, 2017, 837(2): 117. (期刊论文)
(7)Tong, Hao*; Pulsar braking: magnetodipole vs. wind,Science China-Physics Mechanics & Astronomy, 2016, 59(1): 5972. (期刊论文)
(8) Ou, Z. W.;Tong, H.*; Kou, F. F.; Ding, G. Q.; Fluctuating neutron star magnetosphere: braking indices of eight pulsars, frequency second derivatives of 222 pulsars and 15 magnetars ,Monthly Notices of the Royal Astronomical Society, 2016, 457(4): 3922-3933. (期刊论文)
(9)Tong, H.*; The anti-glitch of magnetar 1e 2259+586 in the wind braking scenario,Astrophysical Journal, 2014, 784(2): 86. (期刊论文)
(10)Tong, H.*; Xu, R. X.; SGR 0418+5729: a small inclination angle resulting in a not so low dipole magnetic field?,Astrophysical Journal Letters, 2012, 757(1): L10.(期刊论文)
(11)Tong, H.*; Song, L. M.; Xu, R. X.; Anomalous X-ray pulsars and soft gamma-ray repeaters in the outer gap model: confronting Fermi observations,Astrophysical Journal, 2011, 738(1): 31. (期刊论文)
(12)Tong, H.*; Song, L. M.; Xu, R. X.; Non-detection in a Fermi/LAT observation of AXP 4U 0142+61: magnetars?,Astrophysical Journal Letters, 2010, 725(2): L196. (期刊论文)
