4.7 Article

Population properties and multimessenger prospects of neutron star-black hole mergers following GWTC-3

Related references

Note: Only part of the references are listed.
Review Physics, Particles & Fields

Rates of compact object coalescences

Ilya Mandel et al.

Summary: Gravitational-wave detections enable measurements of the frequency of coalescence of compact objects, such as neutron stars and black holes. Electromagnetic observations and theoretical models further constrain the coalescence rate of binary systems containing neutron stars.

LIVING REVIEWS IN RELATIVITY (2022)

Article Astronomy & Astrophysics

The effect of spin mismodelling on gravitational-wave measurements of the binary neutron star mass distribution

Sylvia Biscoveanu et al.

Summary: The mass distribution of binary neutron stars derived from gravitational-wave observations can provide important insights, but ignoring the spin distribution may introduce biases in the inferred mass distribution. Introducing a prior that matches the true spin distribution can reduce these biases.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2022)

Article Astronomy & Astrophysics

Constraints on compact binary merger evolution from spin-orbit misalignment in gravitational-wave observations

B. P. Gompertz et al.

Summary: The confirmation of the first neutron star-black hole (NS-BH) binary mergers by the LIGO, Virgo, and KAGRA collaboration allows for further investigation into these events. The tilt angle of the black hole's spin relative to the binary's orbital angular momentum vector is discussed, along with the implications for the physical processes that determine this tilt. The early sample of NS-BH events suggests efficient mass transfer and the possibility of more massive NS-BH binaries merging before completing their evolution. Future gravitational-wave detections are predicted to continue displaying similar total binary masses and mass ratios. However, a high mass candidate event may imply a dynamical capture origin, and large tilts in merging NS-BH systems would hinder electromagnetic detection prospects.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2022)

Article Astronomy & Astrophysics

Population Properties of Gravitational-wave Neutron Star-Black Hole Mergers

Jin-Ping Zhu et al.

Summary: By analyzing the gravitational-wave NSBH candidates, researchers have investigated the mass and spin distributions of NSBH mergers. The primary black hole mass distribution in NSBH systems is consistent with previous studies on binary black hole systems, while the neutron star mass spectrum shows a nearly flat distribution. Additionally, the spins of the discovered NSBH mergers are found to be almost zero, implying that most events in the universe are plunging events. Further observations will provide more insights into the population properties of cosmological NSBH mergers.

ASTROPHYSICAL JOURNAL (2022)

Article Astronomy & Astrophysics

A Channel to Form Fast-spinning Black Hole-Neutron Star Binary Mergers as Multimessenger Sources

Rui-Chong Hu et al.

Summary: The study examines the formation and properties of neutron star-black hole binaries, suggesting a promising scenario where neutron stars are born first as multimessenger sources. It highlights the crucial role of fast-spinning black holes in tidal disruption events, and discusses the potentiality of tidal disruption events associated with these systems.

ASTROPHYSICAL JOURNAL (2022)

Article Astronomy & Astrophysics

Kilonova Detectability with Wide-field Instruments

Eve A. Chase et al.

Summary: Kilonovae are transient events in the ultraviolet, optical, and infrared spectrum powered by radioactive decay of heavy elements following a neutron star merger. Joint observations of kilonovae and gravitational waves can provide important constraints for understanding the origin of heavy elements in the Galaxy. This study quantifies the capabilities of different wide-field-of-view instruments to detect kilonovae and explores the variation in detectability with different properties of the kilonova ejecta.

ASTROPHYSICAL JOURNAL (2022)

Article Astronomy & Astrophysics

Modelling the formation of the first two neutron star-black hole mergers, GW200105 and GW200115: metallicity, chirp masses, and merger remnant spins

Debatri Chattopadhyay et al.

Summary: The isolated binary evolution of two neutron star-black hole systems is studied using a grid of population synthesis models. The results suggest that these systems may originate from stars with lower metallicity. Chirp mass and remnant spins are found to be useful in constraining the models, while the effective spin parameter does not provide additional information. Distinguishable features in the distribution of remnant spin parameters are observed in different sub-populations.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2022)

Article Astronomy & Astrophysics

Universal Relations for the Increase in the Mass and Radius of a Rotating Neutron Star

Andreas Konstantinou et al.

Summary: Rotation affects a neutron star's mass and radius, but not its equation of state. Measurements of rotating neutron stars can be used to infer the mass and radius of nonrotating neutron stars. The changes in polar and equatorial radii exhibit symmetry.

ASTROPHYSICAL JOURNAL (2022)

Article Astronomy & Astrophysics

Bridging the Gap: Categorizing Gravitational-wave Events at the Transition between Neutron Stars and Black Holes

Amanda Farah et al.

Summary: We analyze gravitational wave data and find evidence for two populations of compact objects, indicating the transition between neutron stars and black holes. We also uncover hints of a lower mass gap between the most massive neutron stars and the least massive black holes. This research has significant implications for understanding the properties and evolution of compact objects.

ASTROPHYSICAL JOURNAL (2022)

Article Astronomy & Astrophysics

Inferring the Neutron Star Maximum Mass and Lower Mass Gap in Neutron Star-Black Hole Systems with Spin

Christine Ye et al.

Summary: Gravitational-wave detections of merging neutron star-black hole systems provide insights into the mass distributions of astrophysical neutron stars and black holes. The study focuses on the maximum neutron star mass, minimum black hole mass, and possible mass gap between them. Rapidly spinning neutron stars may have larger maximum masses compared to nonspinning ones. The research suggests the existence of a mass gap and the minimum mass of a black hole. Future observations could further constrain the maximum nonspinning neutron star mass and determine the relationship between neutron star spin and maximum mass solely from gravitational-wave data. To avoid bias, the spins and masses of rapidly rotating neutron stars need to be modeled simultaneously.

ASTROPHYSICAL JOURNAL (2022)

Article Astronomy & Astrophysics

Linking the rates of neutron star binaries and short gamma-ray bursts

Nikhil Sarin et al.

Summary: This study calculates the fraction of observable short gamma-ray bursts produced through different channels and provides constraints on the merger rates of binary neutron star (BNS) and neutron star-black hole (NSBH) mergers. The study also predicts future constraints for gravitational-wave detections and discusses their implications for understanding the physics of short gamma-ray bursts and binary evolution.

PHYSICAL REVIEW D (2022)

Article Astronomy & Astrophysics

The Challenges Ahead for Multimessenger Analyses of Gravitational Waves and Kilonova: A Case Study on GW190425

Geert Raaijmakers et al.

Summary: In recent years, significant advances have been made in multimessenger astronomy, allowing for joint analyses of gravitational wave and electromagnetic data to provide additional constraints on the fundamental properties of binary progenitors and merger remnants. A new Bayesian framework has been proposed to allow inference of these properties while considering systematic modeling uncertainties. Enhanced mapping between binary progenitor and outflow properties, along with an increase in the quantity and quality of electromagnetic data, is necessary to break degeneracies in the fundamental source parameters.

ASTROPHYSICAL JOURNAL (2021)

Article Astronomy & Astrophysics

Black Hole Gravitational Potential Enhanced Fallback Accretion onto the Nascent Lighter Compact Object: Tentative Evidence in the O3 Run Data of LIGO/Virgo

Shao-Peng Tang et al.

Summary: The gravitational potential of the primary black hole in a binary system may enhance fallback accretion onto the lighter compact object formed in the second supernova explosion. Recent suggestions propose that final masses of binary compact objects are correlated. Analysis of four gravitational-wave events with a small mass ratio and low mass of the lighter component shows tentative evidence for mass correlation among the objects. Simulations with a mock population and Bayesian hierarchical inference suggest that with dozens of low mass ratio events, the existence of mass correlation in component mass distributions can be robustly tested and accurately determined.

ASTROPHYSICAL JOURNAL (2021)

Article Astronomy & Astrophysics

Black-hole-Neutron-star Mergers Are Unlikely Multimessenger Sources

Giacomo Fragione

Summary: The study conducted a statistical analysis of binary stars forming BH-NS binaries and found that a high-spinning BH and stiff NS EOS increase the likelihood of an electromagnetic counterpart; however, current observational constraints reduce the potential for BH-NS mergers as multimessenger sources.

ASTROPHYSICAL JOURNAL LETTERS (2021)

Article Astronomy & Astrophysics

GW200115: A Nonspinning Black Hole-Neutron Star Merger

Ilya Mandel et al.

Summary: GW200115 represents the second confident detection of the merger between a black hole and a neutron star through gravitational waves. The study indicates a large black hole spin misaligned with the orbital angular momentum and suggests that a nonspinning binary system is more consistent with current astrophysical understanding.

ASTROPHYSICAL JOURNAL LETTERS (2021)

Article Astronomy & Astrophysics

The Mass Distribution of Neutron Stars in Gravitational-wave Binaries

Philippe Landry et al.

Summary: Utilizing gravitational wave observations, the study provides the first inference of the mass distribution of extragalactic neutron star population, revealing that the neutron stars in gravitational-wave binaries follow a uniform distribution with a higher prevalence of high-mass neutron stars. The maximum mass in the gravitational-wave population aligns with expectations from neutron stars in our Galaxy and dense matter.

ASTROPHYSICAL JOURNAL LETTERS (2021)

Article Astronomy & Astrophysics

Formation of the First Two Black Hole-Neutron Star Mergers (GW200115 and GW200105) from Isolated Binary Evolution

Floor S. Broekgaarden et al.

Summary: The study shows that the first two observed BHNS mergers can be explained through the isolated binary evolution channel for reasonable model realizations. Most model realizations can account for the local BHNS merger rate densities inferred by LIGO-Virgo, but to match other systems' merger rate densities as well, models with specific parameters are needed.

ASTROPHYSICAL JOURNAL LETTERS (2021)

Article Astronomy & Astrophysics

The Relative Contribution to Heavy Metals Production from Binary Neutron Star Mergers and Neutron Star-Black Hole Mergers

Hsin-Yu Chen et al.

Summary: The study used gravitational wave detection results, improved neutron star EoS measurements, and advanced numerical simulations to measure the contributions of NSBH and BNS to the production of heavy elements. It found that BNS has produced more r-process elements than NSBH over the past 2.5 billion years in most scenarios. Additionally, if black hole spins are small and there is a lack of low-mass black holes in NSBH binaries, BNS can account for almost all r-process elements in binary systems.

ASTROPHYSICAL JOURNAL LETTERS (2021)

Article Astronomy & Astrophysics

One Channel to Rule Them All? Constraining the Origins of Binary Black Holes Using Multiple Formation Pathways

Michael Zevin et al.

Summary: The study analyzed the second batch of LIGO-Virgo gravitational wave catalog using five binary black hole population models, finding that multiple formation channels contribute to the observed sample of binary black holes and no single channel dominates the detections. Results also showed a preference for natal spins of isolated black holes less than or equal to 0.1 and common-envelope efficiencies of around 2.0.

ASTROPHYSICAL JOURNAL (2021)

Article Astronomy & Astrophysics

The Role of Core-collapse Physics in the Observability of Black Hole Neutron Star Mergers as Multimessenger Sources

Jaime Roman-Garza et al.

Summary: Recent 1D core-collapse simulations show a non-monotonic relationship between the explosivity of massive stars and their precollapse core masses, affecting the formation of coalescing black hole-neutron star binaries significantly. Direct collapse leading to low-mass black holes increases BH-NS merger detection rates, with the NS radius and equation of state influencing the likelihood of electromagnetic counterparts being produced. Models based on 1D core-collapse simulations predict a higher ratio of BH-NS mergers to binary BHs, but may overestimate the local merger density rate of binary black holes.

ASTROPHYSICAL JOURNAL LETTERS (2021)

Article Astronomy & Astrophysics

Population Properties of Compact Objects from the Second LIGO-Virgo Gravitational-Wave Transient Catalog

R. Abbott et al.

Summary: The study reveals unique characteristics of the merging binary black hole (BBH) population, including a specific primary mass spectrum and misaligned component spins leading to precession of the orbital plane. The research also estimates merger rates, indicating potential correlation between BBH rate and redshift but not exceeding the star formation rate. Additionally, recent exceptional events are examined in relation to population models, with GW190814 being identified as an outlier due to its low secondary mass.

ASTROPHYSICAL JOURNAL LETTERS (2021)

Article Astronomy & Astrophysics

Modelling neutron star-black hole binaries: future pulsar surveys and gravitational wave detectors

Debatri Chattopadhyay et al.

Summary: This study models the formation and evolution of neutron star-black hole binaries, predicting the number of observable binaries in the galaxy and discussing the potential for observation by next-generation radio telescopes and gravitational wave detectors. Systems where the neutron star formed first can be distinguished from those where the black hole formed first based on their properties.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2021)

Article Physics, Multidisciplinary

Prospects for Measuring the Hubble Constant with Neutron-Star-Black-Hole Mergers

Stephen M. Feeney et al.

Summary: Gravitational wave and electromagnetic observations of neutron-star-black-hole mergers can provide precise local measurements of the Hubble constant, with achievable unbiased estimates of 1.5%-2.4% precision by 2030. However, the achievable precision is strongly affected by the details of spin precession and tidal disruption, highlighting the need for improved modeling of NSBH mergers.

PHYSICAL REVIEW LETTERS (2021)

Review Astronomy & Astrophysics

Observational Constraints on Black Hole Spin

Christopher S. Reynolds

Summary: The spin of black holes is a crucial aspect to understanding their formation, growth, and energy sources. Current techniques can detect and measure spins at various accretion rates, revealing rapidly spinning supermassive and stellar-mass black holes. Advances in gravitational wave astronomy have provided new insights into spin effects of merging binary black holes, showing a diversity in formation mechanisms between different populations of black holes.

ANNUAL REVIEW OF ASTRONOMY AND ASTROPHYSICS, VOL 59 (2021)

Article Astronomy & Astrophysics

Observation of Gravitational Waves from Two Neutron Star-Black Hole Coalescences

R. Abbott et al.

Summary: This study reports the observation of gravitational waves from two compact binary coalescences in LIGO's and Virgo's third observing run, with properties consistent with neutron star-black hole (NSBH) binaries. The study provides detailed information on the source component masses, source luminosity distances, and more for the two events observed.

ASTROPHYSICAL JOURNAL LETTERS (2021)

Article Astronomy & Astrophysics

Evidence for Hierarchical Black Hole Mergers in the Second LIGO-Virgo Gravitational Wave Catalog

Chase Kimball et al.

Summary: The study indicates compelling evidence for hierarchical mergers in clusters with escape velocities greater than or similar to 100 km/s, with strong support for the hierarchical model over an alternative model with no hierarchical mergers.

ASTROPHYSICAL JOURNAL LETTERS (2021)

Article Astronomy & Astrophysics

Refined Mass and Geometric Measurements of the High-mass PSR J0740+6620

E. Fonseca et al.

Summary: The study reports continued timing observations of PSR J0740+6620, confirming the pulsar mass and properties of the white dwarf companion, and discusses relativistic effects and variations in the orbital period using statistical methods.

ASTROPHYSICAL JOURNAL LETTERS (2021)

Article Astronomy & Astrophysics

Impact of massive binary star and cosmic evolution on gravitational wave observations I: black hole-neutron star mergers

Floor S. Broekgaarden et al.

Summary: Mergers of black hole-neutron star binaries have been observed by gravitational wave detectors, with predicted local BHNS merger rates ranging from 4-830 Gpc(-3) yr(-1). The predictions are significantly impacted by binary evolution and metallicity-specific star formation rate density.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2021)

Article Astronomy & Astrophysics

New insights on binary black hole formation channels after GWTC-2: young star clusters versus isolated binaries

Yann Bouffanais et al.

Summary: With the recent release of the Second Gravitational Wave Transient Catalog (GWTC-2), we are at a turning point of gravitational wave astronomy, able to directly infer constraints on the astrophysical population of compact objects. The study on the origin of binary black hole mergers found that the dynamical model is slightly favored over the isolated model, and parameters have a significant impact on the model inference.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2021)

Article Astronomy & Astrophysics

Impact of the PSR J0740+6620 radius constraint on the properties of high-density matter

Isaac Legred et al.

Summary: The X-ray pulse profile modeling of PSR J0740+6620 using data from NICER and XMM-Newton observatories has led to a measurement of its radius, providing insight into the neutron star equation of state (EoS). The analysis mildly disfavors EoSs supporting a disconnected hybrid star branch and reveals core matter with strong interactions violating the conformal sound-speed bound. Results suggest a relatively stiff EoS and limit the density range probed by observations of cold, non-rotating neutron stars in beta-equilibrium.

PHYSICAL REVIEW D (2021)

Article Astronomy & Astrophysics

Statistical and systematic uncertainties in extracting the source properties of neutron star-black hole binaries with gravitational waves

Yiwen Huang et al.

Summary: The study found that at a network signal-to-noise ratio (SNR) of 30, statistical uncertainties are usually larger than systematic offsets, while at an SNR of 70, the two become comparable. Individual black hole and neutron star masses, as well as mass ratios, are typically measured very precisely, though not always accurately at high SNR. Additionally, the research also indicates that the measurements of neutron star tidal deformability and spin are typically only bounded within a certain range.

PHYSICAL REVIEW D (2021)

Article Astronomy & Astrophysics

Relativistic Shapiro delay measurements of an extremely massive millisecond pulsar

H. T. Cromartie et al.

NATURE ASTRONOMY (2020)

Article Astronomy & Astrophysics

DYNESTY: a dynamic nested sampling package for estimating Bayesian posteriors and evidences

Joshua S. Speagle

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2020)

Article Astronomy & Astrophysics

Bayesian inference for compact binary coalescences with BILBY: validation and application to the first LIGO Virgo gravitational-wave transient catalogue

I. M. Romero-Shaw et al.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2020)

Article Astronomy & Astrophysics

A lower bound on the maximum mass if the secondary in GW190814 was once a rapidly spinning neutron star

Elias R. Most et al.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2020)

Article Astronomy & Astrophysics

Localization of Compact Binary Sources with Second-generation Gravitational-wave Interferometer Networks

Chris Pankow et al.

ASTROPHYSICAL JOURNAL (2020)

Article Astronomy & Astrophysics

GW190425: Observation of a Compact Binary Coalescence with Total Mass ∼3.4 M⊙

B. P. Abbott et al.

ASTROPHYSICAL JOURNAL LETTERS (2020)

Article Astronomy & Astrophysics

Picky Partners: The Pairing of Component Masses in Binary Black Hole Mergers

Maya Fishbach et al.

ASTROPHYSICAL JOURNAL LETTERS (2020)

Article Astronomy & Astrophysics

On the Rate of Neutron Star Binary Mergers from Globular Clusters

Claire S. Ye et al.

ASTROPHYSICAL JOURNAL LETTERS (2020)

Article Physics, Nuclear

Effects of the equation of state on the bulk properties of maximally rotating neutron stars

P. S. Koliogiannis et al.

PHYSICAL REVIEW C (2020)

Article Astronomy & Astrophysics

The heavier the better: how to constrain mass ratios and spins of high-mass neutron star mergers

Elias R. Most et al.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2020)

Article Astronomy & Astrophysics

Slowing the spins of stellar cores

Jim Fuller et al.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2019)

Article Astronomy & Astrophysics

Extracting distribution parameters from multiple uncertain observations with selection biases

Ilya Mandel et al.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2019)

Article Astronomy & Astrophysics

Multimessenger Bayesian parameter inference of a binary neutron star merger

Michael W. Coughlin et al.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2019)

Article Astronomy & Astrophysics

Parallelized inference for gravitational-wave astronomy

Colm Talbot et al.

PHYSICAL REVIEW D (2019)

Article Astronomy & Astrophysics

Reconstructing phenomenological distributions of compact binaries via gravitational wave observations

Daniel Wysocki et al.

PHYSICAL REVIEW D (2019)

Article Astronomy & Astrophysics

Most Black Holes Are Born Very Slowly Rotating

Jim Fuller et al.

ASTROPHYSICAL JOURNAL LETTERS (2019)

Article Astronomy & Astrophysics

BILBY: A User-friendly Bayesian Inference Library for Gravitational-wave Astronomy

Gregory Ashton et al.

ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES (2019)

Article Astronomy & Astrophysics

Can a black hole-neutron star merger explain GW170817, AT2017gfo, and GRB170817A?

Michael W. Coughlin et al.

PHYSICAL REVIEW D (2019)

Review Astronomy & Astrophysics

An introduction to Bayesian inference in gravitational-wave astronomy: Parameter estimation, model selection, and hierarchical models

Eric Thrane et al.

PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF AUSTRALIA (2019)

Article Astronomy & Astrophysics

The spin of the second-born black hole in coalescing binary black holes

Y. Qin et al.

ASTRONOMY & ASTROPHYSICS (2018)

Article Astronomy & Astrophysics

The spin of the second-born black hole in coalescing binary black holes

Y. Qin et al.

ASTRONOMY & ASTROPHYSICS (2018)

Article Astronomy & Astrophysics

The Origin of r-process Elements in the Milky Way

Benoit Cote et al.

ASTROPHYSICAL JOURNAL (2018)

Article Physics, Multidisciplinary

GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral

B. P. Abbott et al.

PHYSICAL REVIEW LETTERS (2017)

Article Astronomy & Astrophysics

Where Are LIGO's Big Black Holes?

Maya Fishbach et al.

ASTROPHYSICAL JOURNAL LETTERS (2017)

Article Astronomy & Astrophysics

Dynamics, nucleosynthesis, and kilonova signature of black hole-neutron star merger ejecta

Rodrigo Fernandez et al.

CLASSICAL AND QUANTUM GRAVITY (2017)

Article Astronomy & Astrophysics

The effect of pair-instability mass loss on black-hole mergers

K. Belczynski et al.

ASTRONOMY & ASTROPHYSICS (2016)

Article Astronomy & Astrophysics

Maximum mass, moment of inertia and compactness of relativistic stars

Cosima Breu et al.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2016)

Article Astronomy & Astrophysics

The effect of pair-instability mass loss on black-hole mergers

K. Belczynski et al.

ASTRONOMY & ASTROPHYSICS (2016)

Article Astronomy & Astrophysics

MODELS OF KILONOVA/MACRONOVA EMISSION FROM BLACK HOLE-NEUTRON STAR MERGERS

Kyohei Kawaguchi et al.

ASTROPHYSICAL JOURNAL (2016)

Article Astronomy & Astrophysics

Advanced LIGO

J. Aasi et al.

CLASSICAL AND QUANTUM GRAVITY (2015)

Article Astronomy & Astrophysics

Fast rotating neutron stars with realistic nuclear matter equation of state

F. Cipolletta et al.

PHYSICAL REVIEW D (2015)

Article Astronomy & Astrophysics

Advanced Virgo: a second-generation interferometric gravitational wave detector

F. Acernese et al.

CLASSICAL AND QUANTUM GRAVITY (2015)

Article Astronomy & Astrophysics

RELATIVISTIC SIMULATIONS OF BLACK HOLE-NEUTRON STAR COALESCENCE: THE JET EMERGES

Vasileios Paschalidis et al.

ASTROPHYSICAL JOURNAL LETTERS (2015)

Article Astronomy & Astrophysics

RADIOACTIVELY POWERED EMISSION FROM BLACK HOLE-NEUTRON STAR MERGERS

Masaomi Tanaka et al.

ASTROPHYSICAL JOURNAL (2014)

Article Astronomy & Astrophysics

RADIATIVE TRANSFER SIMULATIONS OF NEUTRON STAR MERGER EJECTA

Masaomi Tanaka et al.

ASTROPHYSICAL JOURNAL (2013)

Article Multidisciplinary Sciences

A Massive Pulsar in a Compact Relativistic Binary

John Antoniadis et al.

SCIENCE (2013)

Article Astronomy & Astrophysics

WHAT IS THE MOST PROMISING ELECTROMAGNETIC COUNTERPART OF A NEUTRON STAR BINARY MERGER?

B. D. Metzger et al.

ASTROPHYSICAL JOURNAL (2012)

Article Astronomy & Astrophysics

Extracting equation of state parameters from black hole-neutron star mergers: Nonspinning black holes

Benjamin D. Lackey et al.

PHYSICAL REVIEW D (2012)

Article Astronomy & Astrophysics

Black-hole-neutron-star mergers: Disk mass predictions

Francois Foucart

PHYSICAL REVIEW D (2012)

Article Astronomy & Astrophysics

Constraints on a phenomenologically parametrized neutron-star equation of state

Jocelyn S. Read et al.

PHYSICAL REVIEW D (2009)

Article Astronomy & Astrophysics

Dynamo action by differential rotation in a stably stratified stellar interior

HC Spruit

ASTRONOMY & ASTROPHYSICS (2002)

Article Astronomy & Astrophysics

The nucleosynthetic signature of Population III

A Heger et al.

ASTROPHYSICAL JOURNAL (2002)