|
| 04/26/02
| |
Sol Helene |
Observatoire de Paris |
| Place J. Janssen | SF2A- PNG- ASHRA- PCHE- |
|
92295 |
Meudon, France |
Presentation 1 : Poster
Zooming towards Active Galactic Nuclei (PNG)
Woillez, J, Sol, H., Lai, O, Perrin, G.
The advent of large interferometers in the infrared and optical ranges
(VLTI, KI, OHANA) will soon open a new window on AGN compact cores,
accretion and ejection features, gas, dust and stellar content of
galactic nuclei. Simple models of nuclear jets, broad line regions,
circumnuclear disks and starbursts are necessary to interpret the
expected interferometric parameters and will allow to constrain AGN
physics.
Presentation 2 : Poster
Modelling the multifrequency emission of blazars (PCHE)
Katarzynski, K., Sol, H., Kus, A.
Synchrotron and inverse-Compton emission from inhomogeneous jets
is quite successful in explaining multifrequency emission of blazars
from low energy radio range to TeV energies, once correction for
contamination by the host galaxy has been applied. In this frame, we
considere two scenarios for VHE flares. Comparison with light
curves obtained in radio and other low frequency range allows some
test of the models, as we show for Mrk 421.