Accessing the innermost regions of Active Galactic Nuclei
Abstract
Description
Very-long-baseline interferometry can image the parsec-scale structure of radio jets, but the accretion disk close to the black hole remains invisible. One way to probe this accretion flow is provided by X-ray flux density monitoring and spectroscopy. Here we report on preliminary results of a multi-band campaign on NGC1052 with the goal of combining both approaches to access to the innermost regions of this active galaxy and to establish a connection between the relativistic jets and the accretion region.
Proc. First Meeting of Spanish Radio Astronomy, eds. J. C. Guirado, I. Marti-Vidal, J. M. Marcaide, Servicio de Publicaciones, Universidad de Valencia; one figure, one table, needs macropere2006.tex
Proc. First Meeting of Spanish Radio Astronomy, eds. J. C. Guirado, I. Marti-Vidal, J. M. Marcaide, Servicio de Publicaciones, Universidad de Valencia; one figure, one table, needs macropere2006.tex