Predictions of the disc instability model
| dc.creator | Schreiber, M. R. | |
| dc.creator | Hameury, J. -M. | |
| dc.creator | Lasota, J. -P. | |
| dc.date | 2004-11-09 | |
| dc.date.accessioned | 2026-07-07T02:15:43Z | |
| dc.date.available | 2026-07-07T02:15:43Z | |
| dc.description | Confronting the predictions of numerical calculations with observations is an important tool to progress with our understanding of the mechanism triggering the outbursts of dwarf novae and soft X-ray transients. Simultaneous multi-wavelength observations are of particular importance in this process as they contain information about the chronology of the outbursts as e.g. the famous UV-delay observed in dwarf novae. We review key-predictions of the disc instability model (DIM) and confront them with the corresponding observations. | |
| dc.description | 6 pages, 3 figures, to appear in The astrophysics of cataclysmic variables and related objects, ASP Conf. Ser., eds. J.-M. Hameury and J.-P. Lasota | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0411228 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0411228 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/8515 | |
| dc.subject | Astrophysics | |
| dc.title | Predictions of the disc instability model | |
| dc.type | text |