スポンサーリンク
Astronomical Institute Graduate School Of Science Tohoku University | 論文
- Lyman Break Galaxies at z - 5 : Rest-Frame UV Spectra. II
- CO Observations of a FeLoBAL Quasar with an Hα Absorption Line at z=2.3
- Cosmological Evolution of the Hard X-Ray AGN Luminosity Function : Formation History of Supermassive Black Holes(Session 6 : Formation and Evolution of Black Holes)
- Lyman Break Galaxies at z - 5 : Luminosity Function
- Suzaku Observation of the Ophiuchus Galaxy Cluster : One of the Hottest Cool Core Clusters
- High Metallicity of the X-Ray Gas Up to the Virial Radius of a Binary Cluster of Galaxies : Evidence of Galactic Superwinds at High-Redshift
- Spectropolarimetric Study on Circumstellar Structure of Microquasar LS I + 61°303
- Formation of Intermediate-Mass Black Holes in Circumnuclear Regions of Galaxies
- Deep-Imaging Observations of a Candidate of an Absorbed QSO at z=0.653, AX J131831+3341
- A Geometrical Relationship between Broad-Line Clouds and an Accretion Disk around Active Galactic Nuclei
- A Forming Dwarf Galaxy in a Tidal Tail of the Merging Galaxy NGC 2782
- Detection of Molecular Clouds in the Interarm of the Flocculent Galaxy NGC 5055
- Variation of Molecular Cloud Properties across the Spiral Arm in M 51
- MOIRCS deep survey (7) NIR morphologies of star-forming galaxies at redshift z〜1 (Special issue: Exploring the universe with the Subaru Telescope: from galaxies to the solar system)
- Why Does NGC 1068 Have a More Powerful Active Galactic Nucleus than NGC 4258?
- CO(J=3-2) Observations of MS 1512-cB58 at z=2.72
- Detection of Iron Emission in the z = 5.74 QSO SDSSp J104433.04-012502.2
- Low-Resolution Spectral Classification of Very Faint Emission-Line Galaxies
- On a Growing Transverse Mode as a Post-Newtonian Effect in the Large-Scale Structure Formation : Astrophysics and Relativity
- Non-Radial Pulsation of a Boson Star. I : Formulation : Astrophysics and Relativity