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The jet-disk connection in AGN

Tullia Sbarrato
September 15, 2014

The jet-disk connection in AGN

Talk at the IAU Symposium 313 "Extragalactic Jets from every angles", held in Puerto Ayora (Galapagos Islands, Ecuador)

Tullia Sbarrato

September 15, 2014
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  1. The jet-disc connection in AGN Tullia Sbarrato IAUS313, September 15th

    2014 in collaboration with P. Padovani (ESO) and G. Ghisellini (INAF-OAB) Sbarrato, Padovani & Ghisellini, 2014, MNRAS, accepted [arXiv:1405.4865]
  2. Outline • jet & disc in AGN ➡ how to

    trace them? • studying the jet-disc connection with blazars • we need both blazars and radio-galaxies! • results IAUS313, September 15th 2014
  3. broad line region luminosity: traces photo-ionizing luminosity from optical spectra

    Jet & accretion in AGN IAUS313, September 15th 2014 accretion structure vs. relativistic jet gamma-ray luminosity: traces jet power from gamma-ray telescopes
  4. Accretion structures in AGN IAUS313, September 15th 2014 Mahadevan 1997

    radiatively efficient Shakura-Sunyaev (1973) alpha-disc radiatively inefficient advection-dominated accretion flow (ADAF)
  5. Accretion structures in AGN IAUS313, September 15th 2014 Mahadevan 1997

    radiatively efficient Shakura-Sunyaev (1973) alpha-disc radiatively inefficient advection-dominated accretion flow (ADAF)
  6. broad line region luminosity: traces photo-ionizing luminosity from optical spectra

    Jet & accretion in AGN IAUS313, September 15th 2014 accretion structure vs. relativistic jet
  7. broad line region luminosity: traces photo-ionizing luminosity from optical spectra

    Jet & accretion in AGN IAUS313, September 15th 2014 accretion structure vs. relativistic jet radio luminosity: traces jet power in all jetted AGN! from radio surveys
  8. The jet-disc connection in AGN IAUS313, September 15th 2014 radio-galaxies

    must be beamed: spine-layer structure! Sbarrato et al. 2014
  9. Conclusions • blazars do not allow studies on extremely wide

    accretion ranges: lack of low-accreting blazars • blazars and radio-galaxies together cover the transition between efficient and inefficient accretion regimes • ionizing luminosity in inefficient accretion regime decreases with a slope steeper than Maybe ? IAUS313, September 15th 2014