Speaker
Paolo Padovani
(ESO)
Description
I will present a comprehensive multi-messenger view of NGC 1068, the prototype
Seyfert II galaxy recently associated with high-energy IceCube neutrinos. Various
aspects of the source, including its nuclear activity, jet, outflow, and the
starburst region, will be analised in detail using a multi-wavelength approach.
I will also explore its gamma-ray and neutrino emissions to try to understand
which astrophysical component is responsible for the IceCube neutrinos.
Primary author
Paolo Padovani
(ESO)
