スポンサーリンク
Astronomical Institute, Graduate School of Science, Tohoku University | 論文
- Sub-Parsec-Scale Acceleration of the Radio Jet in the Poweful Radio Galaxy NGC 6251
- ^CO(J=1-0)and ^CO(J=1-0) Mapping of the Starburst Galaxy M82
- Possible Method to Reconstruct the Cosmic Equation of State from Strong Gravitational Lensing Systems
- Stratified Structure of Narrow-Line Regions in Active Galactic Nuclei(Abstracts of Doctoral Dissertations,Annual Report(from April 2003 to March 2004))
- Spectropolarimetric Study on Circumstellar Structure of Microquasar LS I + 61°303
- Formation of Intermediate-Mass Black Holes in Circumnuclear Regions of Galaxies
- A Geometrical Relationship between Broad-Line Clouds and an Accretion Disk around Active Galactic Nuclei
- Why Does NGC 1068 Have a More Powerful Active Galactic Nucleus than NGC 4258?
- Detection of Excess Hard X-Ray Emission from the Optical Jet Galaxy NGC 1097
- A Statistical Study on the Difference between Normal and Starburst Galaxies
- Starburst-AGN Connection : A Lesson from High-z Powerful Radio Galaxies(Session 6 : Formation and Evolution of Black Holes)
- Low-Resolution Spectral Classification of Very Faint Emission-Line Galaxies
- On the Equation of Motion for a Fast Moving Small Object in the Strong Field Point Particle Limit
- Why Can We Detect the High-Redshift Quasar BR 1202-0725 in CO?
- The Most Distant [O III]-Emitting Quasar PKS 1937-101 at Redshift 3.8
- Post-Newtonian Hydrodynamic Equations Using the (3+1) Formalism in General Relativity
- Spectroscopic Diagnostics of Symbiotic Stars : II. Statistical Analyses of Highly Resolved Emission-Line Profiles
- Correlation between Interstellar Polarization and Dust Temperature : Is the Alignment of Grains by Radiative Torques Ubiquitous?