Why Does RZ Leonis Minoris, an Unusual SU UMa Star, Have Such a Short Supercycle?

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概要

• 論文の詳細を見る
• Astronomical Society of Japanの論文
• 1995-06-25

著者

• Osaki Yoji

  Department Of Astronomy School Of Science The University Of Tokyo

関連論文

• A Steady State Model of X-Ray Emitting Coronae around Accreting Non-Magnetic White Dwarfs in Cataclysmic Variables
• Why Does RZ Leonis Minoris, an Unusual SU UMa Star, Have Such a Short Supercycle?
• A Model for WZ Sagittae-Type Dwarf Novae : SU UMa/WZ Sge Connection
• The disk instability model for dwarf nova outbursts
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• Repetitive Rebrightening in the Dwarf Nova EG Cancri
• A Model for a Peculiar SU Ursae Majoris-Type Dwarf Nova ER Ursae Majoris

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