Name: | Gu Minfeng |
---|---|
Position: | Professor |
Phone: | 021-34775314 |
E-mail: | gumf@shao.ac.cn |
Postal Code: | 200030 |
Mailing Address: | 80 Nandan Road, Shanghai |
Resume:
Gu Minfengwas born in Jiangsu province, PRC, 1974. In 1995, he received his BS degree in the Department of Astronomy, Nanjing University. Then, he joined Shanghai Astronomical Observatory (SHAO), CAS. After obtaining a Ph.D. degree in 2002 from SHAO, he worked inKorea Astronomy and Space Science Institute as a postdoctoral fellow (2002-2003).In 2010, he visited University of California, Santa Barbara as a visiting scholar (2010 – 2011). Since 2011, he became a research professor in SHAO.His current research interest is active galactic nuclei, and he has published over 40 SCI papers.
Selected publications:
1、Gu, Minfeng,The evolution of the dusty torus covering factor in quasarsAstrophysical Journal, 2013, 773, 176
2、Gu, M. F.; Li, S. -L.,The ultraviolet/optical variability of steep-spectrum radio quasars: the change in accretion rate?,Astronomy & Astrophysics, 2013, 554, A51
3、Gu, Minfeng; Chen, Yongjun,The compact radio structure of radio-loud narrow line Seyfert 1 galaxies,Astronomical Journal, 2010, 139, 2612
4、Gu, Minfeng; Cao, Xinwu,The anti-correlation between the hard X-ray photon index and the Eddington ratio in low-luminosity active galactic nuclei,Monthly Notices of the Royal Astronomical Society, 2009, 399, 349-356
5、Gu, Minfeng; Cao, Xinwu; Jiang, D. R.,The bulk kinetic power of radio jets in active galactic nuclei,Monthly Notices of the Royal Astronomical Society, 2009, 396, 984
6、Wu, Qingwen; Gu, Minfeng,The X-ray spectral evolution in X-ray binaries and its application to constrain the black hole mass of ultraluminous X-ray sources,Astrophysical Journal, 2008, 682, 212
7、Gu, M.F.; Lee, C.U.; Pak, S.; Yim, H.S.; Fletcher, A.B.,Multi-colour optical monitoring of eight red blazars,Astronomy & Astrophysics, 2006, 450, 39
8、Gu, M.F.; Cao, X.W.; Jiang, D.R.,On the masses of black holes in radio-loud quasars,Monthly Notices of the Royal Astronomical Society, 2001, 327, 1111