Remeis Logo ./bh_blue.jpg
Active Galactic Nuclei
X-ray Continuum Emission and Broad Iron Lines
  • Home
  • Jörn's Teaching Pages
  • Active Galactic Nuclei
    • Introduction
    • History of AGN research
    • AGN Taxonomy
    • Accretion and Accretion Disks
    • X-Ray Detectors
    • X-ray Continuum Emission and Broad Iron Lines
    • Ionization Equilibrium and Line Diagnostics
    • Broad Line Region
    • Narrow Line Region
    • Jets and Radio Loud AGN
    • AGN Surveys and AGN Environment
Introduction
Introduction
AGN X-Ray Continua
AGN X-Ray Continua
Compton Scattering
Thomson Scattering, Compton Scattering
Thermal Comptonization
Energy Exchange, Amplification factor, Spectral shape, Galactic Black Holes
Broad Fe Kalpha Lines
K$\alpha $ Line Diagnostics
Broad Lines with ASCA
MCG$-$6-30-15, Broad Lines with ASCA
Broad Lines with XMM
MCG$-$6-30-15, Other Sources
Debated Cases
Absorption or Lines?
Narrow Lines
Narrow Lines
Conclusions
Conclusions, The Future

Previous  Next
Introduction: IntroductionAGN X-Ray Continua: AGN X-Ray ContinuaCompton Scattering: Thomson ScatteringCompton Scattering: Thomson Scattering
Compton Scattering: Thomson ScatteringCompton Scattering: Thomson ScatteringCompton Scattering: Thomson ScatteringCompton Scattering: Compton Scattering
Compton Scattering: Compton ScatteringCompton Scattering: Compton ScatteringCompton Scattering: Compton ScatteringCompton Scattering: Compton Scattering
Thermal Comptonization: Energy ExchangeThermal Comptonization: Energy ExchangeThermal Comptonization: Energy ExchangeThermal Comptonization: Energy Exchange
Thermal Comptonization: Amplification factorThermal Comptonization: Spectral shapeThermal Comptonization: Spectral shapeThermal Comptonization: Spectral shape
Thermal Comptonization: Spectral shapeThermal Comptonization: Spectral shapeThermal Comptonization: Spectral shapeThermal Comptonization: Spectral shape
Thermal Comptonization: Spectral shapeThermal Comptonization: Spectral shapeThermal Comptonization: Spectral shapeThermal Comptonization: Galactic Black Holes
Broad Fe Kalpha Lines: K$\alpha $ Line DiagnosticsBroad Fe Kalpha Lines: K$\alpha $ Line DiagnosticsBroad Fe Kalpha Lines: K$\alpha $ Line DiagnosticsBroad Fe Kalpha Lines: K$\alpha $ Line Diagnostics
Broad Fe Kalpha Lines: K$\alpha $ Line DiagnosticsBroad Fe Kalpha Lines: K$\alpha $ Line DiagnosticsBroad Fe Kalpha Lines: K$\alpha $ Line DiagnosticsBroad Fe Kalpha Lines: K$\alpha $ Line Diagnostics
Broad Lines with ASCA: MCG$-$6-30-15Broad Lines with ASCA: Broad Lines with ASCABroad Lines with XMM: MCG$-$6-30-15Broad Lines with XMM: MCG$-$6-30-15
Broad Lines with XMM: MCG$-$6-30-15Broad Lines with XMM: MCG$-$6-30-15Broad Lines with XMM: Other SourcesBroad Lines with XMM: Other Sources
Broad Lines with XMM: Other SourcesDebated Cases: Absorption or Lines?Narrow Lines: Narrow LinesNarrow Lines: Narrow Lines
Conclusions: ConclusionsConclusions: ConclusionsConclusions: The FutureConclusions: The Future
Conclusions: The FutureConclusions: The Future 
Previous  Next
 

Valid HTML 4.01! Valid CSS! Last changed 2010 Jun 28
Jörn Wilms / joern.wilms@sternwarte.uni-erlangen.de