[16] Yan, Jingzhi; Zhang, Peng; Liu, Wei; Liu, Qingzhong, "Long-term Optical Studies of the Be/X-Ray Binary RX J0440.9+4431/LS V+44 17", 2016, AJ, 151, 104

[15] Li, Hui; Yan, Jingzhi; Zhou, Jianeng; Liu, Qingzhong, "`Long-term Optical Observations of the Be/X-Ray Binary X Per", 2014, AJ, 148, 113

[14] Yan, J. Z., Li, H., Zhou, J. N., and Liu, Q. Z., ”Multi-wavelength Study of the Be/X-ray Binaries”, 2013, IAUS, 290. 351

[13] Camero-Arranz, A.; Finger, M. H.; Wilson-Hodge, C. A.; Jenke, P.; Steele, I.; Coe, M. J.; Gutierrez-Soto, J.; Kretschmar, P.; Caballero, I.; Yan, J. Z. et al., ”X-Ray and Optical Observations of A 0535+26”, 2012, ApJ, 754, 20

[12] Yan, J. Z., Zuruta Heras, J. A., Chaty, S., Li, H and Liu, Q.Z., ”Multi-wavelength Study of the Be/X-ray Binary: MXB 0656-072”, 2012, ApJ, 753, 73

[11] Yan, J. Z., Li H., and Liu Q.Z., ”Discrete Mass Ejections from the Be/X-ray Binary A0535+26/HD245770”, 2012, ApJ, 744, 37

[10] Liu, Q.Z., Chaty, S., Yan, J. Z., ”Be/X-ray binaries as the progenitors of the supergiant fast X-ray transients IGR J18483-0311 and IGR J11215-5952”, 2011, MNRAS, 415, 3349

[09] Liu Q.Z., Li Hui, Yan, J. Z., ”An alternative evolution scenario for OAO 1657-415 and IGR J18483-0311”, 2010, Science in China, Volume 53, Issue 1, pp.130

[08] Li, H., Yan, J. Z., ”Optical results of the black hole microquasar SS 433”, 2010, Science in China Series G, 53S, 153.

[07] Yan, J. Z., Liu, Q. Z. and Hadrava, P., ”Optical Spectroscopic Observations of Cyg X-1 = HDE 226868”, 2008, AJ, 136, 631.

[06] Yan, J. Z., Liu, Q. Z. and Hang, H. R.,”Optical spectroscopic observations of CI Cam” 2007, AJ, 133, 1478;

[05] Liu, Q. Z., Yan, J. Z., ”Magnetar descendants in HMXBs?”, 2006, AdSpR, 38, 2906.

[04] Yan, J. Z., Liu, Q. Z. and Hang. H. R., ”Long-term spectroscopic and near infrared monitoring of Be/X-ray binaries”, 2007, ChJAA, 6S2, 345(Contribution to the 2005 Lake Hanas International Pulsar Symposium, referred);

[03] Liu, Q. Z., Yan, J. Z., Li, X. D. and Hang, H. R.,”The nature of AX J0051-733 in the SMC: a pulsar born with ultrastrong magnetic field”, 2006, Ap&SS, 2006, 305, 133;

[02] Liu,Q. Z., Yan, J. Z.,”An additional Hα emission component in LS I +61^o303: Further evidence for the Hα emission related to the neutron star” , New Astronomy, 2005, 11, 130;

[01] Yan, J. Z., Liu, Q. Z., and Hang, H. R., ”Preliminary Results of the Optical Observations of Three Microquasars”, ChJAA, 2005, 5S, 247( Contribution to 5th Microquasar Workshop, referred );