2000/11/14 by Fabien Casse, Jonathan Ferreira
Physics and Astronomy · #astro-ph
published as Astrophys.Space Sci. 276 (2001) 263-266 · 4 pages, to be published in the proceeding of the Third Microquasar Workshop, eds A.Castro-Tirado, J. Greiner and J. Paredes
arxiv created 2000/11/14 · arxiv updated 2009/12/01
We present a self-similar, steady-state model describing both a magnetized accretion disc and a magnetohydrodynamic jet. We focus on the role of a hot corona in such a structure. This corona enables the disc to launch various types of jets. By considering the energy conservation, we also present a diagnostic of the luminosity of the magnetized disc, which could explain some observational signatures of galactic objects.