Multi-Band Polarimetry of Be Stars. I. X Persei
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概要
- 論文の詳細を見る
- Astronomical Society of Japanの論文
- 1995-10-25
著者
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HIRATA Ryuko
Department of Astronomy, Faculty of Science, Kyoto University
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KUNJAYA Chatief
Department of Astronomy, Institute of Technology Bandung
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Hirata Ryuko
Department Of Astronomy Faculty Of Science Institute Of Technology Bandung
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Kunjaya Chatief
Department Of Astronomy Faculty Of Science Kyoto University
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- 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
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- 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
- Variable Star Network : World Center for Transient Object Astronomy and Variable Stars
- Interpretation of the Long-Term Variation in Late-Type Active Be Stars
- Multi-Band Polarimetry of Be Stars. I. X Persei
- Variable Star Network : World Center for Transient Object Astronomy and Variable Stars
- Discovery of a Peculiar SU UMa-Type Dwarf Nova ER Ursae Majoris