X-ray Fluctuations from the Slim Disk
| dc.creator | Takeuchi, Mitsuru | |
| dc.date | 2000-05-08 | |
| dc.date.accessioned | 2026-07-07T01:53:25Z | |
| dc.date.available | 2026-07-07T01:53:25Z | |
| dc.description | The responses of perturbations added into the optically thick, advection-dominated accretion disk (ADAD), what we call the slim disk (SD), are investigated through numerical simulations. Although it is proposed that the SD is thermally stable, I find that a perturbation added into the disk is not rapidly damped and moves through the disk in its free-fall time. After the perturbation moves, the global structure of the disk does not vary very much. These facts may account for the substantial variability of the X-ray luminosities of stellar super-luminal jet sources (SLJSs) and Narrow-Line Seyfert 1s (NLS1s). | |
| dc.description | Poster contribution presented at the Joint MPE,AIP,ESO workshop on NLS1s, Bad Honnef, Dec. 1999, to appear in New Astronomy Reviews; also available at http://wave.xray.mpe.mpg.de/conferences/nls1-workshop | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0005162 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0005162 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/961 | |
| dc.subject | Astrophysics | |
| dc.title | X-ray Fluctuations from the Slim Disk | |
| dc.type | text |