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National Astronomical Observatories/Yunnan Observatory, Chinese Academy of Sciences | 論文
- CO J = 3-2 Emission from the "Water Fountain" Sources IRAS 16342-3814 and IRAS 18286-0959
- Orbital Period Changes and Their Explanations in Two Algol Binaries : WY Per and RW Leo
- A Period Investigation of the δ Scuti Star AN Lyncis
- Detection of a Cyclic Period Change in the W UMa-Type System HT Virginis
- An Orbital Period Investigation of the Semi-Detached Near-Contact Binary DD Monocerotis
- CCD Photometric Study of the W UMa-Type Binary II Canis Majoris in the Field of Berkeley 33
- RT Leonis Minoris : Does It Belong to an A- or W-Type Overcontact Binary System?
- CCD Photometric Study of the Contact Binary TX Cnc in the Young Open Cluster NGC 2632
- Photometric Investigations of Three Short-Period Binary Systems : GSC 0763-0572, RR Centauri, and ε Coronae Australis
- On the Period Variation of the Neglected W UMa-type Binary System V714 Monocerotis
- V802 Aquilae : A Short-Period Eclipsing Binary with Magnetic Activity
- The Near-Contact Binary RU Ursae Minoris
- A Period Study of the Near-Contact Binary IR Cassiopeiae
- Parent Distributions of the Periods and Magnetic Inclination Angles of Radio Pulsars
- Photometric Investigation and Possible Light-Time Effect in the Orbital Period of a Marginal Contact System, CW Cassiopeiae
- Is the Evolutionary Outcome of Algol-Type Systems T Leonis Minoris and RW Monocerotis the W UMa Systems?
- An Orbital Period Investigation of the W UMa-Type Binary Y Sextantis
- First R and I Lights and Their Photometric Analyses of GSC 02393-00680
- DM Delphini : A Progenitor of a Contact Binary with a Compact Tertiary Companion
- Light-Curve and Period Changes in the W UMa-Type System TY Bootis