Variability of blazars: probing emission regions and ... - Inaf

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Ultra-rapid variability cm IF Conical geometry cm i.e. inside the BLR Doppler factor is not expected to be > 30 d=0.22 pc = RBLR
Location of VHE emission? Arduous inside BLR! Strong absorption (E>30 GeV within BLR, E>1 TeV outside) (e.g. Liu et al. 2008, Reimer 2007, FT & Mazin 2009, Poutanen & Stern 2010) General Model Decline of the IC scattering efficiency (e.g. Albert et al. 2008, FT & Ghisellini 2008) dependent (not applicabile to hadronic)
Page 1 and 2: Variability of blazars: probe of em
Page 3 and 4: Preamble: setting the stage e - γ
Page 5 and 6: Emission within RBLR Bonnoli et al.
Page 7 and 8: Emission at pc-scale? Variability t
Page 9 and 10: Rapid gamma-ray variability! IF Con
Page 11: The strange case of PKS 1222+216 td
Page 15 and 16: VLBI vapp~14 c Jorstad et al. 2012
Page 17 and 18: Tavecchio et al. 2011
Page 19 and 20: Possibilities to reconcile large d
Page 27 and 28: A joke (?): Photon-axion oscillatio

Variability of blazars: probing emission regions and ... - Inaf

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