|
| | | | |
| | | |
| Stat |
Members: 3645
Articles: 2'504'928
Articles rated: 2609
25 April 2024 |
|
| | | | |
|
Article overview
| |
|
|
Rotational splitting effect in neutron star QPOs | | Lev Titarchuk
; Alex Muslimov
; | | Date: |
27 Aug 1997 | | Subject: | astro-ph | | Abstract: | We explain the peak spacing in the power spectra of millisecond variability detected by the Rossi X-ray Timing Explorer (RXTE) in the X-ray emission from the LMXBs (Sco X-1, 4U1728-34, 4U1608-522, 4U1636-536, etc) in terms of the rotational splitting of an intrinsic frequency (which is of order of the local Keplerian frequency) caused by an accretion disk. We calculate this effect and demonstrate that there is a striking agreement with the observational data. We show that the observed discrete frequencies ranging from 200 to 1200 Hz can be described by a whole set of overtones. For higher overtones (lower frequencies, $lsim $ 100 Hz) the ratio between frequencies is determined by the quantum numbers alone. We suggest that a similar phenomena should be observed in Black Hole (BH) systems for which the QPO (quasi-periodic oscillation) frequency should be inversely proportional to the mass of the compact object. For BH systems the characteristic frequency of oscillations should therefore be a factor of 5-10 less than for a neutron star system. keywords | | Source: | arXiv, astro-ph/9708256 | | Services: | Forum | Review | PDF | Favorites | |
|
|
No review found.
Did you like this article?
Note: answers to reviews or questions about the article must be posted in the forum section.
Authors are not allowed to review their own article. They can use the forum section.
browser Mozilla/5.0 AppleWebKit/537.36 (KHTML, like Gecko; compatible; ClaudeBot/1.0; +claudebot@anthropic.com)
|
| |
|
|
|
|
News, job offers and information for researchers and scientists:
| |
REGISTER