The Accretion-Ejection Instability in X-ray Binaries

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dc.creatorVarniere, P.
dc.creatorTagger, M.
dc.date2000-11-13
dc.date.accessioned2026-07-07T01:56:31Z
dc.date.available2026-07-07T01:56:31Z
dc.descriptionThe Accretion-Ejection Instability (AEI), which can occur in magnetized disks near equipartition, is a good candidate to explain the low-frequency QPO in black-hole binaries. Here we present analytical work concerning the behavior of QPO frequency and the emission of Alfvén waves from the disk to the corona.
dc.description2 pages, 2 color figures, to be published in `Proceedings of the Third Microquasar Workshop: Granada Workshop on galactic relativistic jet sources', Eds A. J.Castro-Tirado, J. Greiner and J. M. Paredes, Astrophysics and Space Science special issue, in press
dc.identifierhttps://arxiv.org/abs/astro-ph/0011247
dc.identifierhttp://arxiv.org/abs/astro-ph/0011247
dc.identifierAstrophys.Space Sci. 276 (2001) 233-234
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/2026
dc.subjectAstrophysics
dc.titleThe Accretion-Ejection Instability in X-ray Binaries
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