Presentation - Active Galactic Nuclei 8 - Inaf

More documents

Recommendations

Info

ParadigmSeyferts:(geometrically) thin accretion diskHigh radiative efficiency (~0.1)-BBB=thermal radiation from AD+Kα EL profile + L/L Edd ~1LINERS: Radiativelyinefficient accretionflows (RIAFs) Ho (2003)-kinetic energyadvected or redirectedinto an outflowP. Romano - AGN8 Meeting - Turin 4
Sample Selection I (Maoz 2005, 2007)17 LINERs UNOBSCUREDknown UV nuclei L(UV)~10 (39-41) erg/sNo dust lanes in optical imagesX-ray absorbing columns are N H
Page 1 and 2: Testing the LINERs paradigmwith Swi
Page 3: Kewley et al. 2006LINERs occupy a w
Page 7 and 8: Maoz et al. 2005, 2007Summary of LI
Page 9 and 10: Swift InstrumentsSpacecraft•Auton
Page 11 and 12: Sample Selection IIIBrightest objec
Page 13 and 14: Swift/XRT data IIM81NGC3998NGC4203N
Page 15 and 16: NGC 3998P. Romano - AGN8 Meeting -
Page 17 and 18: Swift/XRT spectraNo absorptionfeatu
Page 19 and 20: XRT lightcurves IP. Romano - AGN8 M
Page 21 and 22: XRT lightcurves IIIP. Romano - AGN8
Page 23 and 24: Swift/UVOT: uvw1 band images IM81P.
Page 25 and 26: UVOT photometryFlux (10 -15)Galaxyc
Page 27 and 28: Maoz 2007 SEDsP. Romano - AGN8 Meet
Page 29: The EndP. Romano - AGN8 Meeting - T

Presentation - Active Galactic Nuclei 8 - Inaf

Create successful ePaper yourself

Delete template?

Save as template?