Results 1 to 10 of about 131,089 (321)

The Evolution of Compact Binary Star Systems [PDF]

open access: yesLiving Reviews in Relativity, 2014
We review the formation and evolution of compact binary stars consisting of white dwarfs (WDs), neutron stars (NSs), and black holes (BHs). Mergings of compact-star binaries are expected to be the most important sources for forthcoming gravitational-wave
Konstantin A. Postnov, Lev R. Yungelson
doaj   +16 more sources

GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo during the Second Part of the Third Observing Run [PDF]

open access: yesPhysical Review X, 2023
The third Gravitational-Wave Transient Catalog (GWTC-3) describes signals detected with Advanced LIGO and Advanced Virgo up to the end of their third observing run.
R. Abbott   +1657 more
doaj   +2 more sources

Holographic approach to compact stars and their binary mergers [PDF]

open access: yesProgress in Particle and Nuclear Physics, 2021
In this review article, we describe the role of holography in deciphering the physics of dense QCD matter, relevant for the description of compact stars and their binary mergers.
C. Hoyos, Niko Jokela, A. Vuorinen
semanticscholar   +5 more sources

Pre-merger Electromagnetic Counterparts of Binary Compact Stars [PDF]

open access: yesThe Astrophysical Journal, 2018
We investigate emission signatures of binary compact star gravitational wave (GW) sources consisting of strongly magnetized neutron stars (NSs) and/or white dwarfs (WDs) in their late-time inspiral phase.
Jie-Shuang Wang   +3 more
semanticscholar   +5 more sources

Super-Massive Neutron Stars and Compact Binary Millisecond Pulsars [PDF]

open access: yesProceedings of Multifrequency Behaviour of High Energy Cosmic Sources - XIII — PoS(MULTIF2019), 2019
The maximum mass of a neutron star has important implications across multiple research fields, including astrophysics, nuclear physics and gravitational wave astronomy.
M. Linares
semanticscholar   +4 more sources

Mass transfer and evolution of compact binary stars

open access: yes, 2007
. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .
V. Gokhale
semanticscholar   +2 more sources

The Dragon-II simulations - III. Compact binary mergers in clusters with up to 1 million stars: Mass, spin, eccentricity, merger rate and pair instability supernovae rate. [PDF]

open access: yesMonthly notices of the Royal Astronomical Society, 2023
Compact binary mergers forming in star clusters may exhibit distinctive features that can be used to identify them among observed gravitational-wave (GW) sources. Such features likely depend on the host cluster structure and the physics of massive star
M. A. Sedda   +6 more
semanticscholar   +1 more source

The spins of compact objects born from helium stars in binary systems [PDF]

open access: yes, 2022
The angular momentum (AM) content of massive stellar cores helps to determine the natal spin rates of neutron stars and black holes. Asteroseismic measurements of low-mass stars have proven that stellar cores rotate slower than predicted by most prior ...
J. Fuller, Wenbin Lu
semanticscholar   +1 more source

Home - About - Disclaimer - Privacy