Formation of Intermediate-Mass Black Holes in Circumnuclear Regions of Galaxies
スポンサーリンク
概要
- 論文の詳細を見る
- Astronomical Society of Japanの論文
- 2000-06-25
著者
-
TANIGUCHI Yoshiaki
Astronomical Institute, Graduate School of Science, Tohoku University
-
SHIOYA Yasuhiro
Astronomical Institute, Graduate School of Science, Tohoku University
-
Shioya Yasuhiro
Astronomical Institute
-
Shioya Yasuhiro
Astronomical Institute Graduate School Of Science Tohoku University
-
Tsuru Takeshi
Physics Department Graduate School Of Science Kyoto University
-
IKEUCHI Satoru
Physics Department, Graduate School of Science, Nagoya University
-
Taniguchi Yoshiaki
Astronomical Institute Faculty Of Science Tohoku University
-
Taniguchi Yoshiaki
Astronomical Institute Graduate School Of Science Tohoku University
関連論文
- The SUBARU Deep Field Project : Lyman α Emitters at a Redshift of 6.6
- The Subaru Deep Field : The Optical Imaging Data
- A Multi-Band Photometric Study of Tidal Debris in a Compact Group of Galaxies : Seyfert's Sextet
- Molecular Gas in the Poststarburst Galactic Nucleus of NGC 4736
- New Corroborative Evidence for the Overdensity of Galaxies around the Radio-Loud Quasar SDSS J0836 + 0054 at z = 5.8
- Lyα Emitters at z = 5.7 in the Subaru Deep Field
- Strong Emission-Line Galaxies at Low Redshifts in the Field around the Quasar SDSSp J104433.04-012502.2
- An Intermediate-Band Imaging Survey for High-Redshift Lyman Alpha Emitters : The Mahoroba-11
- A Survey of NB921 Dropouts in the Subaru Deep Field
- New High-Redshift Galaxies at z = 5.8-6.5 in the Subaru Deep Field
- The Intermediate-Band Dropout Method : A New Method to Search for High-Redshift Galaxies
- A Subaru Search for Lyman α Emitters at z = 5.8 with an Intermediate-Band Filter
- Are Two z - 6 Quasars Gravitationally Lensed?
- The Discovery of Two Lyman α Emitters beyond Redshift 6 in the Subaru Deep Field
- SDSSp J104433.04-012502.2 at z = 5.74 is Gravitationally Magnified by an Intervening Galaxy
- Decomposition of the Superwind in M 82
- Seyfert-Type Dependences of Narrow Emission-Line Ratios and Physical Properties of High-Ionization Nuclear Emission-Line Regions in Seyfert Galaxies
- High-Resolution Images of the Ring Nebula Taken with the Subaru Telescope
- 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
- 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
- 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
- Tidal Truncation of Gas Replenishment and Global Suppression of Galactic Star Formation in Distant Clusters
- LMSA and High-Redshift Dusty Starburst Mergers
- Chemical Evolution of Disk Galaxies(Abstracts of Doctoral Dissertations,Annual Report (from April 1994 to March 1995))
- Starburst-AGN Connection : A Lesson from High-z Powerful Radio Galaxies(Session 6 : Formation and Evolution of Black Holes)