Reverberation mapping

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Occultation in MCG-6-30-15McKernan & Yaqoob 1998Occultation by optically-thick cloudexplains flux and spectral variabilityin target low state, including Feemission lineDeep dip is aneclipse event !
Partial Covering/Occultation, resurgence of anold ideaAlways an appealingalternative to diskreflection, to explaingeneral shapes of AGNspectra and big fluxvariations (e.g. Boller et al1997, 2002)Explains some Galacticblack holes (e.g. Dower,Bradt, Morgan 1982,Brandt et al 1996, Tanaka,Ueda and Boller 2003)Gierlinski & Done 2004 Turner et al 2007The idea resurfaced with a vengeance because of the complex absorbers revealed by new dataGrating spectroscopy points specifically to a wind origin for the gas
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 and 32: Ambiguity: - X-ray AbsorptionNGC 35
Page 33 and 34: How much evidence is there forabsor
Page 35 and 36: More Evidence for ionized outflows:
Page 37: Seyfert Spectral Variability Behavi
Page 41: Summary• Large amounts of gas are

Reverberation mapping

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