K.-Y. Chen
University of Florida
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Publications of the Astronomical Society of the Pacific | 1988
Maryjane Taylor; K.-Y. Chen; James D. McNeill; John E. Merrill; John P. Oliver; Frank Bradshaw Wood
The authors discuss the results and analysis of 16 hours of continuous photometry of γ2Vel. Indication of a 1.26-hour period of variability in the He II and C III emission lines at 4686 A and 5696 A, respectively, is presented. Although such a period has not been reported by other investigators, recent theoretical studies indicate that such a period may have certain theoretical implications.
Monthly Notices of the Royal Astronomical Society | 1976
K.-Y. Chen; Frank Bradshaw Wood
Archive | 1996
S. P. Robb; K.-Y. Chen; Greg Hudson; Richard L. Hudson; Edwin Budding
Archive | 1992
Edwin Budding; Frank Bradshaw Wood; K.-Y. Chen
Archive | 1992
K.-Y. Chen; Frank Brandshaw Wood; Shu-Yang Jiang; Ji-Tong Zhang; Tong-Sheng Mao; Pei-Sheng Chen; Yu-Lang Yang; Donald H. Martins; Zheng-Hua Yang
Archive | 1992
K.-Y. Chen; Frank Bradshaw Wood
Archive | 1988
Maryjane Taylor; K.-Y. Chen; J. D. McNeill; John E. Merrill; John P. Oliver; Frank Bradshaw Wood
Archive | 1988
John P. Oliver; K.-Y. Chen; Maryjane Taylor; J. D. McNeill; John E. Merrill; Frank Bradshaw Wood
Archive | 1987
Frank Bradshaw Wood; K.-Y. Chen
Archive | 1987
K.-Y. Chen; John P. Oliver; Frank Bradshaw Wood
