Reverberation mapping

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Complex & Variable AbsorptionComponents log ξ~3.5 - 5, N H>> 10 23cm -2 -can we model all curvature withthese?Kallman et al 2004N H~ 3x 10 23 cm -2 , log ξ=2.25Counter claims: Young et al (2005)say cannot thus “explain away”diskline in MCG-6-30-15 strongfeatures ~6.5 keV, not observedHETG, Young et al 2005Counter-counter claims: L. Miller etal (2008) say MCG-6 explainedwithout recourse to blurring
How much evidence is there forabsorption mimicing ‘disklines’• Got to search for absorbing gas in acertain parameter range to get the rightcurvature
Page 1 and 2: Reverberation mappingOptical lines
Page 3 and 4: Reverberation mappingv =GM rGetting
Page 7 and 8: Light Crossing Time•Variations sm
Page 11 and 12: X-ray Observations of AGNWhat we ca
Page 13 and 14: Recap: The Power behind AGNSimple a
Page 15 and 16: Copious production of X-RaysUV phot
Page 17 and 18: X-ray Line ProductionGeorge & Fabia
Page 19 and 20: Chandra/XMMSuzakuAbsorptionfrom out
Page 21 and 22: Profile distorted SR & GR- probe of
Page 23 and 24: GR Effects on Spectral featuresProf
Page 25 and 26: MCG-6-30-15: Poster ChildTanaka et
Page 27 and 28: Absorption or Reflection as the ori
Page 29 and 30: Light bending?Suzaku lightcurveMini
Page 31: Ambiguity: - X-ray AbsorptionNGC 35
Page 35 and 36: More Evidence for ionized outflows:
Page 37 and 38: Seyfert Spectral Variability Behavi
Page 39 and 40: Partial Covering/Occultation, resur
Page 41: Summary• Large amounts of gas are

Reverberation mapping

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