Transient Optical Emission from a Nonstationary Accretion Disk: A Model for Optical Afterglow of Gamma Ray Bursts

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概要

• 論文の詳細を見る
• Astronomical Society of Japanの論文
• 2000-08-25

著者

• CHENG Kwong-Sang

  Department of Physics, University of Hong Kong

• Lu Ye

  Department Of Physics University Of Hong Kong

• Zhao G

  National Astronomical Observatories Chinese Acad. Sci. Beijing Chn

• Cheng Kwong-sang

  Department Of Physics University Of Hong Kong

• Cheng K‐s

  Univ. Hong Kong Hong Kong Chn

• ZHAO Gang

  Beijing Astronomical Observatory, Chinese Academy of Sciences

• Zhao Gang

  Beijing Astronomical Observatory Chinese Academy Of Sciences

関連論文

• Origin of Thermal and Non-Thermal Hard X-Ray Emission from the Galactic Center
• Particle Propagation in the Galactic Center and Spatial Distribution of Non-Thermal X-Rays
• Origin of 6.4keV Line Emission from Molecular Clouds in the Galactic Center
• Transient Optical Emission from a Nonstationary Accretion Disk: A Model for Optical Afterglow of Gamma Ray Bursts
• K-Shell Emission of Neutral Iron Line from Sagittarius B2 Excited by Subrelativistic Protons
• The Multiwavelength Doppler Factors for a Sample of Gamma-Ray Loud Blazars
• A Study on the Orbital Period Variation of AR Lacertae
• Orbital Period Investigation of the RS CVn-Type Binary CG Cygni

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