Issue |
A&A
Volume 423, Number 2, August IV 2004
|
|
---|---|---|
Page(s) | 401 - 404 | |
Section | Astrophysical processes | |
DOI | https://doi.org/10.1051/0004-6361:20035808 | |
Published online | 06 August 2004 |
The MHD Alfven wave oscillation model of kHz Quasi Periodic Oscillations of Accreting X-ray binaries
National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, PR China e-mail: zhangcm@bao.ac.cn Research Center for Theoretical Astrophysics, School of Physics, The University of Sydney, NSW 2006, Australia
Received:
4
December
2003
Accepted:
19
April
2004
We ascribe the interpretation of the twin kilohertz
Quasi Periodic Oscillations (kHz QPOs) of X-ray spectra of Low
Mass X-Ray Binaries (LMXBs) to MHD Alfvén wave oscillations in
the different mass density regions of the accreted matter at the
preferred radius, and the upper kHz QPO frequency
coincides with the Keplerian frequency. The proposed model
concludes that the kHz QPO frequencies depend inversely on the
preferred radius,
and that theoretical relation between the upper frequency () and
the lower frequency (
) is
, which is similar
to the measured empirical relation. The separation between the
twin frequencies decreases (increases) with increasing kHz QPO
frequency if the lower kHz QPO frequency is more (less) than ~400 Hz.
Key words: stars: neutron / X-rays: stars
© ESO, 2004
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