Irradiated Accretion Disk in the Galactic Supersoft X-Ray Source RX J0019.8+2156
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
- 1998-02-25
著者
-
FUKUE Jun
Astronomical Inatitute Osaka Kyoiku University
-
Fukue Jun
Astronomical Institute Osaka Kyoiku University
-
MATSUMOTO Katsura
Department of Astronomy, Faculty of Science, Kyoto University
-
Matsumoto Katsura
Department Of Astronomy Faculty Of Science Kyoto University
関連論文
- Adobe After Effects CS4を用いた動画デジタル教材の自作可能性
- ひらめき・ときめきサイエンス--ようこそ大学の研究室へ 大阪教育大学における3年間の実施報告
- 動画を用いた天文教育普及(4)動画を用いたネット広報活動
- 日本天文学会 早川幸男基金による渡航報告書 : The 2008 Solar Physics Division (SPD) Meeting
- 動画を用いた天文教育普及(3)動画教材の具体例と応用
- "宇宙(天文)を学べる大学"の情報を伝達する戦略を立案するためのアンケート調査
- 動画を用いた天文教育普及(2)動画を用いた天文教育の実際
- 動画を用いた天文教育普及(1)動画を用いた教育の基礎
- Radiation Hydrodynamical Mass Accretion onto Galactic Nuclei Driven by Circumnuclear Starbursts
- Radiative Avalanche Driven by Spherical Starbursts
- Accretion Disks Driven by External Radiation Drag around Central Luminous Sources
- Self-Similar Spherical Accretion via External Radiation Drag
- 天文分野におけるサイエンスデザインの必要性 : 天体の色に関して
- 天体色彩学入門(6)色彩学を用いたサイエンスデザイン(その5)天体をサイエンスデザインする授業
- Spin of Stellar-Mass Black Holes Estimated by a Model of Quasi-Periodic Oscillations
- 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
- Observational Appearance and Spectrum of Black-Hole Winds with Supercritical Accretion Disks
- マイクロレンズを用いた、活動銀河核中心部の分解(重力レンズ現象とHigh-Redshift宇宙,研究会報告)
- Observational Appearance of Relativistic, Spherically Symmetric Massive Winds
- Effect of Radiation Drag on Hoyle-Lyttleton Accretion
- Optical light curves of luminous eclipsing black hole x-ray binaries
- Milne-Eddington Solutions for Relativistic Spherical Flows
- Spherical Relativistic Radiation Flows with Variable Eddington Factor
- Relativistic Radiative Flow in a Luminous Disk II
- Radiative Transfer and Limb Darkening of Accretion Disks
- Relativistic Radiation Hydrodynamical Accretion-Disk Winds
- Black-Hole Winds with a Variable Eddington Factor
- VRI Light Curves of SS 433 : Photometry and Model
- Relativistic Radiative Flow in a Luminous Disk
- Eclipsing Light-Curve Asymmetry for Black-Hole Accretion Flows
- Geometrical Effect of Supercritical Accretion Flows : Observational Implications of Galactic Black-Hole Candidates and Ultraluminous X-Ray Sources
- Sound Speed and the Pseudo-Newtonian Potential
- General Relativity and the Pseudo-Newtonian Potential
- Light-Curve Diagnosis of a Hot Spot for Accretion-Disk Models
- Cloudy Accretion Disks
- Wavy Stratus under Photon Surfing over Luminous Disks
- Line Spectrum from Accretion-Disk Winds
- Winds from the Inner Region of Accretion Disks
- Line Spectrum from Advection-Dominated Accretion Disks
- SUperdisks in Supersoft X-Ray Sources
- Irradiated Accretion Disk in the Galactic Supersoft X-Ray Source RX J0019.8+2156
- Dynamical Stability of Cosmological Accretion Disks Embedded in External Radiation Fields : Optically-Thick Case
- Roche Potential with Luminous Accretion Disks
- Radiative Flow in a Luminous Disk
- Silhouette of a Dressed Black Hole
- Critical Accretion Disk
- Radiative Flow in a Luminous Disk II
- Greenhouse Effect of Cloudy Accretion Disks
- Radiative Transfer in Relativistic Accretion-Disk Winds
- Radiative Transfer in Accretion-Disk Winds
- Terminal Speed of On-Axis Jets from a Supercritical Accretion Disk
- Velocity-Dependent Eddington Factor in Relativistic Radiative Flow
- Radiative Collimation of Electron-Positron Jets II
- Radiato-Magneto-Thermal Winds from an Accretion Disk
- Radiative Collimation of Electron-Positron Jets
- Eclipsing and Precessional Light Curves of SS 433 with Superdisks
- Relativistic Variable Eddington Factor
- B3-4 天文を題材とした科学コミュニケーションを支援する動画教材 : 星のソムリエ[○!R]制度のe-Learning展開へ向けて(セッション8,研究発表:口頭発表)
- Variable Eddington Factor in a Relativistic Plane-Parallel Flow
- Relativistic Spectra of Hot Black-Hole Winds
- Observational Appearance of Black Hole Winds
- Milne-Eddington Solutions for Relativistic Plane-Parallel Flows
- Observational Appearance of Luminous Relativistic Movers
- Configuration and Spectrum of Radiatively-Driven Winds from an Accretion Disk(Poster)
- Light Curve Analysis of Microquasar GRO J1655-40(Poster)
- Relativistic Variable Eddington Factor in a Relativistic Plane-Parallel Flow
- Apparent Photosphere of Massive Accretion-Disk Winds
- Analytical Solutions of Relativistic Plane-Parallel Flows(Astrophysics and Cosmology)
- 第3回「"宇宙(天文)を学べる大学"合同進学説明会」出張オープンキャンパス : 研究室ってどんなとこ?研究者ってどんな人?
- 第2回「"宇宙(天文)を学べる大学"合同進学説明会」 : 広報のあり方
- 見えない影が現れた
- Galactic Black-Hole Candidates Shining at the Eddington Luminosity
- Relativistic Milne-Eddington-Type Solutions with a Variable Eddington Factor for Relativistic Plane-Parallel Flows(Astrophysics and Cosmology)
- Radiative Disk Winds from a Self-Similar Slim Disk
- Dust-Gas Accretion onto a Luminous Object
- Relativistic Radiative Jets Confined by a Disk Corona
- Supercritical Accretion Disks with Superwinds
- Basic Properties of Supercritical Accretion Disks
- Radiative Winds in Supersoft X-Ray Sources with Passive Disks
- Multi-stage Drive of Astrophysical Jets
- Evolution of a Luminous Hoyle-Lyttleton Accretor
- Hoyle-Lyttleton Accretion onto Superdisks
- Bondi Accretion onto a Luminous Object
- Radiative-Thermal Winds from an Accretion Disk
- Light-Curve of a Hot Spot on Advection-Like Accretion Disk(Poster)
- Radiativ Disk Winds under Radiation Drag
- Radiative Disk Winds in Supersoft X-Ray Sources
- Radiative Disk Winds under Radiation Drag II
- We Can See No Naked Supercritical Accretion Disks
- 第4回「"宇宙(天文)を学べる大学"合同進学説明会」出張オープンキャンパス〜研究室ってどんなとこ? 研究者ってどんな人?〜
- Hoyle-Lyttleton Accretion onto Accretion Disks
- Precessional Light Curves of SS 433
- Black-Hole Shadow Has Infinite Optical Depth
- Observational Appearance and Spectrum of Black-Hole Winds
- 第一回2012年金環日食講習会in大阪
- Accretion-Disk Corona Advected by External Radiation Drag I.
- Accretion-Disk Corona Advected by External Radiation Drag II. Relativistic Case
- Accretion Corona Immersed in Disk Radiation Fields