Results 1 to 10 of about 1,454,993 (340)
Проект Байкал, 2021 Baroque and classicism were called a binary star. In the national architecture, the avant-garde and neoclassicism can be also called a binary star. The model of succession of styles in architecture does not reflect the real situation in the 1920-1950s ...
Елена Багина
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Laboratory analogue of a supersonic accretion column in a binary star system. [PDF]
Nat Commun, 2016 Astrophysical flows exhibit rich behaviour resulting from the interplay of different forms of energy—gravitational, thermal, magnetic and radiative. For magnetic cataclysmic variable stars, material from a late, main sequence star is pulled onto a highly
Cross JE +24 more
europepmc +2 more sources
The evolution of binary neutron star post-merger remnants: a review [PDF]
General Relativity and Gravitation, 2021 Two neutron stars merge somewhere in the Universe approximately every 10 to 100 s, creating violent explosions potentially observable in gravitational waves and across the electromagnetic spectrum.
Nikhil Sarin, Paul D. Lasky
openalex +2 more sources
Living Reviews in Relativity, 2012 We review the current status of studies of the coalescence of binary neutron star systems. We begin with a discussion of the formation channels of merging binaries and we discuss the most recent theoretical predictions for merger rates.
Joshua A. Faber, Frederic A. Rasio
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The Evolution of Compact Binary Star Systems [PDF]
Living Reviews in Relativity, 2014 Konstantin A Postnov
exaly +2 more sources
On the Rate of Neutron Star Binary Mergers from Globular Clusters [PDF]
Astrophysical Journal, 2019 The first detection of gravitational waves from a neutron star–neutron star (NS–NS) merger, GW170817, and the increasing number of observations of short gamma-ray bursts have greatly motivated studies of the origins of NS–NS and neutron star–black hole ...
Claire S. Ye +6 more
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Binary black hole mergers from population III stars: uncertainties from star formation and binary star properties [PDF]
Monthly notices of the Royal Astronomical Society, 2023 Population III (Pop. III) binary stars likely produced the first stellar-born binary black hole (BBH) mergers in the Universe. Here, we quantify the main sources of uncertainty for the merger rate density evolution and mass spectrum of Pop. III BBHs by
F. Santoliquido +7 more
semanticscholar +1 more source
Impact of Massive Binary Star and Cosmic Evolution on Gravitational Wave Observations I: Black Hole – Neutron Star Mergers [PDF]
Monthly notices of the Royal Astronomical Society, 2021 Mergers of black hole-neutron star (BHNS) binaries have now been observed by GW detectors with the recent announcement of GW200105 and GW200115.
F. Broekgaarden +9 more
semanticscholar +1 more source
Gaia Data Release 3. Astrometric binary star processing [PDF]
Astronomy & Astrophysics, 2022 Context.The Gaia Early Data Release 3 contained the positions, parallaxes and proper motions of 1.5 billion sources, among which some did not fit well the"single star"model. Binarity is one of the causes of this. Aims.
J. Halbwachs +8 more
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Impact of massive binary star and cosmic evolution on gravitational wave observations II: Double compact object rates and properties [PDF]
Monthly notices of the Royal Astronomical Society, 2021 Making the most of the rapidly increasing population of gravitational-wave detections of BH and NS mergers requires comparing observations with population synthesis predictions. In this work we investigate the combined impact from the key uncertainties
F. Broekgaarden +11 more
semanticscholar +1 more source