矮新星爆発の統一モデル
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矮新星爆発の統一モデル
尾崎洋二, 1994.2
- Title Transcription
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ワイシンセイ バクハツ ノ トウイツ モデル
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研究分担者:柴橋博資
平成4,5年度科学研究費補助金(一般研究C)研究成果報告書,研究課題番号:04640267
Contents of Works
- Time evolution of the accretion disk radius in a Dwarf nova / S. Ichikawa[ほか]
- Ginga observation of SS Cygni / K. Yoshida[ほか]
- Superoutburst and superhump phenomena in SU Ursae Majoris stars : enhanced mass-transfer episode or pure disk phenomenon? / S. Ichikawa[ほか]
- Superhump periods in SU Ursae Majoris stars : eigenfrequency of the eccentric mode of an accretion disk / M. Hirose[ほか]
- Self-consistent accretion disk-coronal model for active galactic nuclei / K. Nakamura[ほか]
- Superoutburst and superhump phenomena of SU Ursa Majoris stars
- Tidal effects on accretion disks in close binary systems
- Disk instability model for SU UMa stars : SU UMa/WZ Sge connection
- Recurrence time for dwarf nova outbursts : dependence on mass transfer rate / S. Ichikawa[ほか]
- A self-consistent accretion disk-coronal model for the active galactic nuclei / K. Nakamura[ほか]