The Accretion-Ejection Instability and a "Magnetic Flood" scenario for GRS 1915+105
| dc.creator | Tagger, Michel | |
| dc.date | 2000-11-15 | |
| dc.date.accessioned | 2026-07-07T01:56:32Z | |
| dc.date.available | 2026-07-07T01:56:32Z | |
| dc.description | I present a global view of recent results on the Accretion-Ejection Instability (AEI), described in more details in other contributions to this workshop. These results address essentially the characteristics of the AEI as a good candidate to explain the low-frequency QPO of X-ray binaries, in particular (at $\sim 1-10$ Hz) of micro-quasars. I then discuss how, if the AEI is considered as the source of the QPO, a possible scenario can be considered where the $\sim 30$ mn. cycles of GRS 1915+105 are controlled by the evolution of magnetic flux in the disk. | |
| dc.description | 4 pages, 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, in press | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0011300 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0011300 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/2036 | |
| dc.subject | Astrophysics | |
| dc.title | The Accretion-Ejection Instability and a "Magnetic Flood" scenario for GRS 1915+105 | |
| dc.type | text |