  M 87 is the first extragalactic source detected in the Very High Energy (VHE;
E > 100 GeV) gamma-ray domain that is not a blazar, its large scale jet not
being aligned to the line of sight. Slight modification of standard emission
models of TeV blazars allows to account for the gamma-ray spectra obtained with
H.E.S.S. We present a multi-blob synchrotron self-Compton model taking
explicitly into account large viewing angles and moderate values of the Lorentz
factor as inferred from MHD simulations of jet formation. Predictions of the
VHE emission for the nearby radiogalaxy Cen A and an interpretation of the
broadband radiation of M 87 are presented.
