| Education and Career History |
B.S. 1983, Dalian University of Technology, China M.S. 1986, Dalian University of Technology, China PhD. 2000, The University of Hong Kong, China 1986-1995, Hebei University of Technology, China 1998-2001, RA, Sao Paulo State University, Brazil 2001-2004, RA, The University of Sydney, Australia 2004-now, National Astronomical Observatories, China |
| Research Fields |
Pulsar astrophysics, X-ray neutron star in binary system, ISM and radio pulsar scintillation, kHz QPOs of LMXBs, General relativity |
| Achievements |
Dedicated to the neutron star magnetic field evolution, and spin formation and evolution of millisecond pulsar, the mechanism of kHz QPOs of LMXB, |
| Selected Publication |
(1) Y. Yang，C.M. Zhang，D. Li，et al.，Similarity of PSR J1906+0746 to PSR J0737–3039: a Candidate of a New Double Pulsar System?，The Astrophysical Journal，2017.01.30 (2) D. H. Wang，C. M. Zhang，Y. J. Lei，et al., Probing the accretion disc structure by the twin kHz QPOs and spins of neutron stars in LMXBs，Monthly Notices of the Royal Astronomical Society，2017.01.05 (3) Y. Y. Pan，L. M. Song，C. M. Zhang，H. Tong，The magnetic field evolution of ULX NuSTAR J095551+6940.8 in M82–a legacy of an accreting magnetar, MNRAS，2016.04.29 (4) Y. Q. Guo, C. M. Zhang，Y. Y. Pan，The spin period formation of millisecond pulsar by the torques of accretion and gravitational wave emission，Astrophysics and Space Science，2016.10.17 (5) D.H. Wang，L. Chen, C.M.Zhang，Investigation of the emission radii of kHz QPOs for the accretingmillisecond X-Ray pulsars, Atoll and Z sources，MNRAS，2015.01.01 (6) C.M. Zhang, T.M. Belloni， M. Mendez, S.N. Zhang, 2013, editors of "Feeding Compact Objects -- Accretion on All Scales" (Proceedings of IAUS290), Cambridge University Press, UK |
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