Accessing the innermost regions of Active Galactic Nuclei
| dc.creator | Ros, E. | |
| dc.creator | Kadler, M. | |
| dc.date | 2006-08-21 | |
| dc.date.accessioned | 2026-07-07T07:19:24Z | |
| dc.date.available | 2026-07-07T07:19:24Z | |
| dc.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. | |
| dc.description | 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 | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0608424 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0608424 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/114610 | |
| dc.subject | Astrophysics | |
| dc.title | Accessing the innermost regions of Active Galactic Nuclei | |
| dc.type | text |