Binary and Millisecond Pulsars

Abstract

We review the main properties, demographics and applications of binary and millisecond radio pulsars. Our knowledge of these exciting objects has greatly increased in recent years, mainly due to successful surveys which have brought the known pulsar population to over 1800. There are now 83 binary and millisecond pulsars associated with the disk of our Galaxy, and a further 140 pulsars in 26 of the Galactic globular clusters. Recent highlights include the discovery of the young relativistic binary system PSR J1906+0746, a rejuvination in globular cluster pulsar research including growing numbers of pulsars with masses in excess of 1.5 solar masses, a precise measurement of relativistic spin precession in the double pulsar system and a Galactic millisecond pulsar in an eccentric (e=0.44) orbit around an unevolved companion.

Available on-line at http://www.livingreviews.org/lrr-2008-8

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• Modeling Mergers of Known Galactic Systems of Binary Neutron Stars
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• Post-Newtonian Kozai-Lidov Mechanism and its Effect on Cumulative Shift of Periastron Time of Binary Pulsar
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• Probing Ensemble Properties of Vortex-avalanche Pulsar Glitches with a Stochastic Gravitational-Wave Background Search
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• Assessment of a new sub-grid model for magnetohydrodynamical turbulence. II. Kelvin-Helmholtz instability
• Bayesian sensitivity of binary pulsars to ultra-light dark matter
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• Reducing the number of templates for aligned-spin compact binary coalescence gravitational wave searches using metric-agnostic template nudging
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• On the spin period distribution of millisecond pulsars
• Radio Millisecond pulsars
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• Halo millisecond pulsars ejected by intermediate mass black holes in globular clusters
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• A NICER View of Spectral and Profile Evolution for Three X-ray Emitting Millisecond Pulsars
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• Propagation of gravitational waves in multimetric gravity
• Slowly-Rotating Neutron Stars in Massive Bigravity
• Inferring small neutron star spins with neutron star-black hole mergers
• Observational evidence for a spin-up line in the P-Pdot diagram of millisecond pulsars
• Population study for gamma-ray pulsars; II Millisecond pulsars
• Eccentric millisecond pulsars by resonant convection
• Physical Environment of Accreting Neutron Stars
• Vela Pulsar: Single Pulses Analysis with Machine Learning Techniques
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• Defining Millisecond Pulsars
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• Testing the Accretion-induced Field-decay and Spin-up Model for Recycled Pulsars
• Methods for relativistic self-gravitating fluids: From binary neutron stars to black hole-disks and magnetized rotating neutron stars
• The End of the Rainbow: What Can We Say About the Extragalactic Sub-Megahertz Radio Sky?
• LB-1 is inconsistent with the X-ray source population and pulsar-black hole binary searches in the Milky Way
• The impact of a stochastic gravitational-wave background on pulsar timing parameters
• Investigation of the Millisecond Pulsar Origins by their Spin Periods at the Wavebands of Radio, X-Ray, and γ-Ray
• The MAVERIC Survey: The first radio and X-ray limits on the detached black holes in NGC 3201
• A Strange Star Scenario for the Formation of Eccentric Millisecond Pulsar PSR J1946+3417
• Accretion, Ablation and Propeller Evolution in Close Millisecond Pulsar Binary Systems
• A Search for Millisecond-pulsar Radio Emission from the Faint Quiescent Soft X-ray Transient 1H 1905+000
• Prediction of radio-quiet gamma-ray pulsar distances using the Fundamental Plane relation
• Fourier Domain
• Estimates of the Surface Magnetic Field Strength of Radio Pulsars
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• Constraining light fermionic dark matter with binary pulsars
• A simple, flexible method for timing cross-calibration of space missions
• Optimizing the low-latency localization of gravitational waves
• The micro-glitch in PSR B1821-24 : A case for a strange pulsar?
• Enhanced particle acceleration in a pulsar wind interacting with a companion
• TRAPUM pulsar and transient search in the Sextans A and B galaxies and discovery of background FRB 20210924D
• On the Gravitational Wave Counterpart to a Gamma-ray Galactic Center Signal from Millisecond Pulsars
• Challenges in Forming Millisecond Pulsar-Black Holes from Isolated Binaries
• Impact of magnetic field gradients on the development of the MRI: Applications to binary neutron star mergers and proto-planetary disks
• Probing Picohertz Gravitational Waves with Pulsars
• Pulsars and Millisecond Pulsars II: Deep diving into the Evolutionary Mechanisms
• Formation of millisecond pulsars with wide orbits
• Quark Novae: An Alternative Channel For the Formation of Isolated Millisecond Pulsars
• Scintillation Bandwidth Measurements from 23 Pulsars from the AO327 Survey
• Pulsar Timing Constraints on Cumulative and Individual Mass of Stars in the Galactic Center
• Neutron Star as a Mirror for Gravitational Waves
• Possible tidal dissipation in millisecond pulsar binaries
• Constraints on Population I/II neutron star-black hole binary formation by gravitational wave and radio observations
• Isolated neutron stars and studies of their interiors
• Astronomy and the new SI
• Radio polarization of millisecond pulsars with multipolar magnetic fields
• Compact binary system dynamics at the second post-Newtonian order: analytical formula of the coordinate time for eccentric and circular orbits
• Nano-Hertz Gravitational Waves Searches with Interferometric Pulsar Timing Experiments
• Radio pulse search from Aql X-1
• General relativistic magnetohydrodynamics simulations for binary neutron star mergers
• Search of nearby resolved neutron stars among optical sources
• On the Formation of Eccentric Millisecond Pulsars by Accretion-induced Collapse of Massive White Dwarfs
• Application of Efron-Petrosian method to radio pulsar fluxes
• Millisecond Pulsars in Globular Clusters and Implications for the Galactic Center Gamma-Ray Excess
• A deep Chandra study verifies diffuse non-thermal X-ray emission from the globular cluster Terzan 5
• Thermal and Magnetic effects on Bulk Viscosity in Binary Neutron Star Mergers
• The contribution to Galactic Centre γ-ray excess from cluster-born millisecond pulsars. Constraints from direct N-body simulations
• Upper limits on microhertz gravitational waves from supermassive black-hole binaries using PSR J1909-3744 data from the second IPTA data release
• GRB 130603B: No Compelling Evidence For Neutron Star Merger
• Timing Gravity with Pulsars in the Strong Field
• High performance Stingray
• Probing fundamental physics with pulsars