QPOs in 4U 1626-67

Details QPOs in 4U 1626-67 QPOs in 4U 1626-67

Dec 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997atel....1....1k&link_type=abstract

The Astronomer's Telegram, #1

Astronomy and Astrophysics

Astronomy

3

X-Ray, Binaries, Pulsars

Scientific paper

The low-mass X-ray binary pulsar 4U 1626-67 shows quasi-periodic oscillations (QPOs) with a centroid frequency of 0.048 Hz and red noise variability as well as coherent pulsations at the 0.130 Hz neutron star rotation frequency. In power density spectra of observations made with the Rossi X-ray Timing Explorer, we have found significant sidebands at the frequencies (n*f_0 - f_qpo) and (n*f_0 + f_qpo), where f_0 = 0.130 Hz is the pulsar spin frequency, f_qpo = 0.048 Hz is the QPO frequency, and n = 1,2,3...

Affiliated with

Also associated with

No associations

Rating

QPOs in 4U 1626-67 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 QPOs in 4U 1626-67, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and QPOs in 4U 1626-67 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-892534