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MHD jets around galactic objects

Fabien Casse·Jonathan Ferreira
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Abstract

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.

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Fabien Casse, Jonathan Ferreira. 2000-11-14. MHD jets around galactic objects. https://arxiv.org/abs/astro-ph/0011264

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