DISCOVERY OF THE QUASI-PERIODIC OSCILLATIONS FROM V0332+53
Citation
T. Takeshima et al., DISCOVERY OF THE QUASI-PERIODIC OSCILLATIONS FROM V0332+53, The Astrophysical journal, 436(2), 1994, pp. 871-874
Categorie Soggetti
Astronomy & Astrophysics
SICI code
0004-637X(1994)436:2<871:DOTQOF>2.0.ZU;2-V
Abstract
The discovery of quasi-periodic oscillations (QPOs) in the X-ray flux
from the recurrent transient X-ray pulsar V0332+53 is reported. The ce
ntroid frequency, full width at half-maximum (FWHM), and the relative
root mean square (rms) amplitude of the QPOs are (5.1 +/- 0.5) x 10(-2
) Hz, (3.3 +/- 1.5) x 10(-2) Hz, and 4.8% +/- 1.2%, respectively. The
beat frequency model is tested using these results and previously repo
rted QPOs from other X-ray binary pulsars.