Interpretation of the Long-Term Variation in Late-Type Active Be Stars

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概要

• 論文の詳細を見る
• Astronomical Society of Japanの論文
• 1995-04-25

著者

• HIRATA Ryuko

  Department of Astronomy, Faculty of Science, Kyoto University

• Hirata Ryuko

  Department Of Astronomy Faculty Of Science Kyoto University

• Hirata Ryuko

  Department Of Astronomy Faculty Of Science Institute Of Technology Bandung

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• Galactic Rotation Derived from OB Stars Using Hipparcos Proper Motions and Radial Velocities
• Non-LTE Calculation for the Be Star Decretion Disk
• Forty Years of Spectroscopic Stellar Astrophysics in Japan
• Period Analysis of the Radial Velocity in Pleione
• Discovery of a New SU UMa-Type Dwarf Nova, V 1028 Cygni
• Spectroscopic and Photometric Observations of a Z Cam-Type Dwarf Nova, AT Cancri, in Standstill
• Discovery of a Large-Amplitude SU UMa-Type Dwarf Nova, CT Hydrae
• Discovery of a New SU UMa-Type Dwarf Nova, V1113 Cygni
• Photometric Observations of an Extreme ER UMa Star, RZ Leonis Minoris
• HV Virginis and WZ Sge-Type Dwarf Novae
• Maximum Visible Polarization of 4179 Toutatis in the Apparition of 1996
• Interpretation of the Long-Term Variation in Late-Type Active Be Stars
• Multi-Band Polarimetry of Be Stars. I. X Persei

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