THE FORMATION OF THE ECCENTRIC-ORBIT MILLISECOND PULSAR J1903+0327 AND THE ORIGIN OF SINGLE MILLISECOND PULSARS

Binary and Millisecond Pulsars

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MASS TRANSFER IN BINARY STARS USING SMOOTHED PARTICLE HYDRODYNAMICS. I. NUMERICAL METHOD

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MASS TRANSFER IN BINARY STARS USING SMOOTHED PARTICLE HYDRODYNAMICS. II. ECCENTRIC BINARIES

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ADIABATIC MASS LOSS IN BINARY STARS. I. COMPUTATIONAL METHOD

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FURTHER EVIDENCE FOR THE BIMODAL DISTRIBUTION OF NEUTRON-STAR MASSES

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ADIABATIC MASS LOSS AND THE OUTCOME OF THE COMMON ENVELOPE PHASE OF BINARY EVOLUTION

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Can eccentric binary millisecond pulsars form by accretion-induced collapse of white dwarfs?

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The low-mass X-ray binary-millisecond radio pulsar birthrate problem revisited

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A FURTHER DROP INTO QUIESCENCE BY THE ECLIPSING NEUTRON STAR 4U 2129+47

(2009) Jinrong Lin et al.   ASTROPHYSICAL JOURNAL

A FALLBACK DISK ACCRETION INVOLVED FORMATION CHANNEL TO PSR J1903+0327

(2009) Xi-Wei Liu et al.   ASTROPHYSICAL JOURNAL

A Radio Pulsar/X-ray Binary Link

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Spectroscopic observations of the quiescent neutron star system 4U 2129+47 (=V1727 Cygni)

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A catalogue of multiplicity among bright stellar systems

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A multiphysics and multiscale software environment for modeling astrophysical systems

(2008) Simon Portegies Zwart et al.   NEW ASTRONOMY

An Eccentric Binary Millisecond Pulsar in the Galactic Plane

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