The bottom magnetic field and magnetosphere evolution of neutron star in low-mass X-ray binary [PDF]
Monthly Notices of the Royal Astronomical Society, 2006 8 pages, 4 figs, accepted by MNRAS ...
Yasufumi Kojima, Cheng-Min Zhang
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THE MASS AND THE RADIUS OF THE NEUTRON STAR IN THE TRANSIENT LOW-MASS X-RAY BINARY SAX J1748.9–2021 [PDF]
The Astrophysical Journal, 2013 Accepted for publication in the Astrophysical Journal ...
Feryal Özel, Feryal Özel, Tolga Guver
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Evolving Neutron Star Low-Mass X-ray Binaries to Ulta-compact X-ray Binaries
, 2010 7pages, 3figures. To appear in Proceedings for "Compact stars in the QCD phase diagram II (CSQCD II), May 20-24, 2009, KIAA at Peking University, Beijing - P. R. China [http://vega.bac.pku.edu.cn/rxxu/csqcd.htm]
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Cooling of the Crust in the Neutron Star Low-Mass X-Ray Binary MXB 1659-29
The Astrophysical Journal, 2008 In quasi-persistent neutron star transients, long outbursts cause the neutron star crust to be heated out of thermal equilibrium with the rest of the star. During quiescence, the crust then cools back down. Such crustal cooling has been observed in two quasi-persistent sources: KS 1731-260 and MXB 1659-29.
Jon M. Miller +4 more
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Reflecting on accretion in neutron star low-mass X-ray binaries
Astrophysics and Space ScienceComment: Accepted for publication in Astrophysics and Space Science, 11 pages (+9 pages for references), 6 ...
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A study of accretion discs around rapidly rotating neutron stars in general relativity and its applications to four low mass X–ray binaries [PDF]
, 2002 Sudip Bhattacharyya
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Observational signatures of neutron stars in low-mass X-ray binaries climbing a stability peak [PDF]
, 2015 E. M. Kantor +2 more
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Kilohertz QPOs in low-mass X-ray binaries as oscillation modes of tori around neutron stars – I [PDF]
, 2017 Márcio G. B. de Avellar +3 more
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Silicon K-edge Dust Properties of Neutron Star Low-mass X-ray Binaries
Proceedings of the International Astronomical Union, 2020 AbstractThe dust properties of the line-of-sight materials in neutron star low-mass X-ray binaries (LMXBs) can be probed by X-ray observations and laboratory experiments. We use a Markov chain Monte Carlo (MCMC) method to conduct a spectral analysis of Chandra ACIS-S/HETG archival data of a sample of LMXBs, including GX 5-1 and GX 13+1.
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Bounds on Compactness for Low‐Mass X‐Ray Binary Neutron Stars from X‐Ray Burst Oscillations [PDF]
, 2002 Nitya Nath +2 more
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