Presentation - Active Galactic Nuclei 8 - Inaf
Presentation - Active Galactic Nuclei 8 - Inaf
Presentation - Active Galactic Nuclei 8 - Inaf
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Maoz et al. 2005, 2007Summary of LINER monitoring campaign:Most LINERs vary in the UV on short timescales, long timescales, orboth. At least some of UV is nonstellar.Variable UV flux gives lower limit on AGN component of UV luminosity– can constrain SED/ accretion modeScaled down versions of SeyfertsSeyfertsLINERsP. Romano - AGN8 Meeting - Turin 7
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