スポンサーリンク
Astronomical Institute, Osaka Kyoiku University | 論文
- How Do We See a Relativistic Accretion Disk during a Thermal Instability?
- Self-Similar Solutions for ADAF with Toroidal Magnetic Fields
- Radiatively-Driven Relativistic Accretion Disk Winds
- Discovery of Multiple High-Velocity Narrow Circumstellar Na I D Lines in Nova V1280 Sco
- Determination of Hydrogen Peroxide by High-Performance Liquid Chromatography with a Cation-Exchange Resin Gel Column and Electrochemical Detector
- Optical and Near-Infrared Photometry of Nova V2362 Cyg : Rebrightening Event and Dust Formation
- Anti-Correlation of Near-Infrared and X-Ray Variations of the Microquasar GRS 1915+105 in the Soft State
- The 2006 November Outburst of EG Aquarii : the SU UMa Nature Revealed
- Discovery of a WZ Sge-Type Dwarf Nova, SDSS J102146.44+234926.3 : Unprecedented Infrared Activity during a Rebrightening Phase
- Observational Appearance of Relativistic, Spherically Symmetric Massive Winds
- High-Dispersion Spectra Collection of Nearby F-K Stars at Okayama Astrophysical Observatory : A Basis for Spectroscopic Abundance Standards
- High Dispersion Spectrograph (HDS) for the Subaru Telescope
- Forty Years of Spectroscopic Stellar Astrophysics in Japan
- Dramatic Spectral and Photometric Changes of Pleione (28 Tau) between 2005 November and 2007 April
- Discovery of a New SU UMa-Type Dwarf Nova, V 1028 Cygni
- Photometric Observations of an Extreme ER UMa Star, RZ Leonis Minoris
- Sulfur Abundances in Metal-Poor Stars Based on OAO-1.88m/HIDES Spectra
- On Black Hole Mass Estimation from X-Ray Spectra of Ultraluminous X-Ray Sources
- Spherical Relativistic Radiation Flows with Variable Eddington Factor
- Relativistic Radiative Flow in a Luminous Disk II