Implications of kHz quasi-periodic brightness oscillations in X-ray binaries for neutron star structure
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/302/4/L69/18634161/302-4-L69.pdf
Reference23 articles.
1. A Microscopic Interpretation of Neutron Star Structure
2. Dense baryon matter calculations with realistic potentials
3. Formation and evolution of binary and millisecond radio pulsars
Cited by 5 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. Ways to constrain neutron star equation of state models using relativistic disc lines;Monthly Notices of the Royal Astronomical Society;2011-06-07
2. Measurement of neutron star parameters: A review of methods for low-mass X-ray binaries;Advances in Space Research;2010-04
3. Millisecond Oscillations in X-Ray Binaries;Annual Review of Astronomy and Astrophysics;2000-09
4. Bounds on neutron-star moments of inertia and the evidence for general relativistic frame dragging;Physical Review D;1999-12-16
5. Quasi-periodic oscillations in low-mass X-ray binaries and constraints on the equation of state of neutron star matter;Monthly Notices of the Royal Astronomical Society;1999-09-23
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