Discovery of the quasi-periodic oscillations from V0332+53

Details Discovery of the quasi-periodic oscillations from V0332+53 Discovery of the quasi-periodic oscillations from V0332+53

Dec 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994apj...436..871t&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 436, no. 2, p. 871-874

Astronomy and Astrophysics

Astronomy

34

Pulsars, Spaceborne Astronomy, Stellar Models, Stellar Oscillations, X Ray Astronomy, X Ray Binaries, Astronomical Spectroscopy, Ginga Satellite, Mathematical Models, X Ray Spectra

Scientific paper

The discovery of quasi-periodic oscillations (QPOs) in the X-ray flux from the recurrent transient X-ray pulsar VO332+53 is reported. The centroid 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 reported QPOs from other X-ray binary pulsars.

Affiliated with

Also associated with

No associations

Rating

Discovery of the quasi-periodic oscillations from V0332+53 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Discovery of the quasi-periodic oscillations from V0332+53, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Discovery of the quasi-periodic oscillations from V0332+53 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1326118