The statistics of Sco X-1 kHZ QPOs
| dc.creator | Bulik, Tomasz | |
| dc.date | 2005-10-13 | |
| dc.date.accessioned | 2026-07-07T06:43:51Z | |
| dc.date.available | 2026-07-07T06:43:51Z | |
| dc.description | Recently an additional technique was applied to investigate the properties of kHz QPOS, i.e. the analysis of the distribution of frequency ratios or frequencies themselves. I review the results of such work on the data from ScoX-1: Abramowicz et al. (2003), which was later criticized by Belloni et al.(2005). I conclude that the findings of the latter paper are consistent with results presented earlier: kHz QPOs cluster around the value corresponding to the frequency ratio of 2/3. I also discuss the random walk model of kHz QPOs and possible future observations needed to verify it. | |
| dc.description | Astronomische Nachrichten, in press | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0510388 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0510388 | |
| dc.identifier | Astron.Nachr. 326 (2005) 861-863 | |
| dc.identifier | doi:10.1002/asna.200510418 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/102576 | |
| dc.subject | Astrophysics | |
| dc.title | The statistics of Sco X-1 kHZ QPOs | |
| dc.type | text |