Models of quasi-periodic variability in neutron stars and black holes-Reference-Cited by-同舟云学术

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Models of quasi-periodic variability in neutron stars and black holes

Published:2001-01 Issue:2-3 Volume:28 Page:481-491
ISSN:0273-1177
Container-title:Advances in Space Research
language:en
Short-container-title:Advances in Space Research

Author:

Psaltis D.

Publisher

Elsevier BV

Subject

Space and Planetary Science,Aerospace Engineering,General Earth and Planetary Sciences,Atmospheric Science,Geophysics,Astronomy and Astrophysics

Reference33 articles.

1. A note on the geometrical thickness of the accretion flow close to the black hole;Abramowicz;PASJ,1985

2. Model QPO power spectra - Signatures of angular position and radial velocity of clumps in the boundary layer;Alpar;MNRAS,1986

3. Is GX 5—1 a millisecond pulsar?;Alpar;Nature,1985

4. Towards a Unified Description of the Timing Features of Accreting Neutron Stars and Black Holes;Belloni;ApJ,2000

5. Rotational Evolution during Type I X-Ray Bursts;Cumming;ApJ,2000

Cited by 16 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Lags of the kilohertz quasi-periodic oscillations in the transient source XTE J1701−462;Monthly Notices of the Royal Astronomical Society;2022-04-19

2. Rotating stars in relativity;Living Reviews in Relativity;2017-11-29

3. The impact of neutron star spin on X-ray spectra;Monthly Notices of the Royal Astronomical Society;2017-11-01

4. Lense-Thirring Precession in the Astrophysical Context;Probing The Nature of Gravity;2010

5. Lense-Thirring Precession in the Astrophysical Context;Space Science Reviews;2009-12

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