TeVブレーザーの多波長スペクトルを用いた物理状態の考察(プラズマと宇宙ジェット,21世紀を迎える理論天文学の総括と展望,研究会報告)
スポンサーリンク
概要
- 論文の詳細を見る
Using multi-frequency spectra from TeV blazars in quiescent states, we obtain the physical parameters of the emission region of blazars, based on the synchrotron self-Compton model. We numerically calculate the steady-state electron energy spectrum by self-consistently taking into account radiative cooling effects with a proper account of the Klein-Nishina effects. We find that for Mrk 421, Mrk 501, and PKS 2155-304, the energy density of magnetic fields is about one order of magnitude less than that of relativistic electrons, which confirms the previous claim made analytically.
- 素粒子論グループ 素粒子研究編集部の論文
- 2001-07-20
著者
-
TAKAHARA Fumio
Department of Earth and Space Science, Graduate School of Science, Osaka University
-
Takahara Fumio
Department Of Earth And Space Science Graduate School Of Science Osaka University
-
紀 基樹
阪大理
-
KUSUNOSE Masaaki
Department of Physics, School of Science, Kwansei Gakuin University
-
Kusunose Masaaki
Department Of Physics School Of Science Kwansei Gakuin University
-
Kusunose Masaaki
Department Of Astronomy University Of Tokyo
-
Kusunose M
Department Of Physics School Of Science Kwansei Gakuin University
関連論文
- Suzaku Observation of Diffuse X-Ray Emission from the Open Cluster Westerlund 2 : a Hypernova Remnant?
- Giant Flare of SGR 1806-20 from a Relativistic Jet
- Photon Emission in a Cascade from Relativistic Protons Initiated by Residual Thermal Photons in Gamma-Ray Bursts
- On Radiative Acceleration of Relativistic Jets : Astrophysics and Relativity
- The Spectral Index of Accelerated Particles in Shock Waves with Oblique Magnetic Field
- Cosmological Reionization Caused by Structure Formation : Astrophysics and Relativity
- A Simple Model of Cosmological Reionization : Astrophysics and Relativity
- Optically Thin, Advection-Dominated Two-Temperature Disks
- Global Structures of Advection-Dominated Two-Temperature Accretion Disks
- TeVブレーザーの多波長スペクトルを用いた物理状態の考察(プラズマと宇宙ジェット,21世紀を迎える理論天文学の総括と展望,研究会報告)
- Electron-Positron Pair Equilibrium in a Mildly Relativistic Plasma : Effects of the Comptonization of Soft Photons : Astrophysics and Relativity
- Electron-Positron Pair Production in a Hot Accretion Plasma around a Massive Black Hole : Astrophysics and Relativity
- The Electron Spectrum in 3C 279 and the Klein-Nishina Effects(Poster)
- Pair Equilibrium in a Relativistic Plasma with Magnetic Fields
- Collective Instabilities of Self-Gravitating Systems. III : Disk-Halo System
- Collective Instabilities of Self-Gravitating Systems. II : Instabilities Due to Temperature Anisotropy
- Collective Instabilities of Self-Gravitating Systems : Infinite Homogeneous Case
- Dynamical Collapse of the Intracluster Gas and the Formation of a Hot Plasma in Clusters of Galaxies
- On the Origin of Galactic TeV Unidentified Sources(Chapter 6. SN1006 Milenium Special Session, The Extreme Universe in the Suzaku Era)
- 降積円盤からのX線スペクトル(X線とγ線,理論天文学の新展開-大型観測計画とともに,研究会報告)
- Global Relationships among the Physical Properties of Galaxy Cluster Cores
- Episodic Accretion onto Neutron Stars and Cosmic Gamma-Ray Bursts
- Effect of Rayleigh Scattering on Cosmic Microwave Background Anisotropies : Astrophysics and Relativity
- X-Ray Emission from Active Galactic Nuclei : Comptonization of Self-Absorbed Cyclotron Higher Harmonics
- On the Chemical Evolution of Our Galaxy
- On the Origin of Highest Energy Cosmic Rays : Progress Letters
- A Magnetized Accretion Disk Model of Quasars and Active Galactic Nuclei
- Magnetic Flare Model of Quasars and Active Galactic Nuclei : Magnetized Accretion Disk around a Massive Black Hole
- On the Origin and Evolution of the Intracluster Gas : Interaction with Galaxies
- Global Stability of the Uniformly Rotating Gaseous Disks
- The Electron Spectrum in 3C 279 and the Klein-Nishina Effects(Poster)
- Hydrostatic Structure of a Hot Plasma in a Cluster of Galaxiers