GRS 1915+105: Ten Years After
| dc.creator | Belloni, Tomaso | |
| dc.date | 2002-08-06 | |
| dc.date.accessioned | 2026-07-07T02:04:36Z | |
| dc.date.available | 2026-07-07T02:04:36Z | |
| dc.description | It is now ten years since the first microquasar GRS 1915+105 was discovered. More than six years of observations with RossiXTE have shown a level of variability never observed in any other X-ray source. Here I try to address some issues, based on X-ray observations only, that have relevance for theoretical modeling. First, I ignore these peculiarities and concentrate on the similarities with other X-ray transients. Then I focus on the peculiar variability and present a number of obervational facts that need to be addressed by theoretical models. | |
| dc.description | 8 pages, 8 figures; to appear in Proceedings of the 4th Microquasar Workshop, eds. Ph Durouchoux, Y. Fuchs and J. Rodriguez, published by the Center for Space Physics: Kolkata | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0208129 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0208129 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/4819 | |
| dc.subject | Astrophysics | |
| dc.title | GRS 1915+105: Ten Years After | |
| dc.type | text |