MHD jets around galactic objects

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dc.creatorCasse, Fabien
dc.creatorFerreira, Jonathan
dc.date2000-11-14
dc.date.accessioned2026-07-07T01:56:31Z
dc.date.available2026-07-07T01:56:31Z
dc.descriptionWe 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.
dc.description4 pages, to be published in the proceeding of the Third Microquasar Workshop, eds A.Castro-Tirado, J. Greiner and J. Paredes
dc.identifierhttps://arxiv.org/abs/astro-ph/0011264
dc.identifierhttp://arxiv.org/abs/astro-ph/0011264
dc.identifierAstrophys.Space Sci. 276 (2001) 263-266
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/2029
dc.subjectAstrophysics
dc.titleMHD jets around galactic objects
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