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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   +14 more sources

Nucleosynthesis of Binary-stripped Stars

open access: yesThe Astrophysical Journal, 2023
The cosmic origin of the elements, the fundamental chemical building blocks of the universe, is still uncertain. Binary interactions play a key role in the evolution of many massive stars, yet their impact on chemical yields is poorly understood.
R. Farmer   +4 more
doaj   +4 more sources

Fast rotating stars resulting from binary evolution will often appear to be single [PDF]

open access: yes, 2010
Rapidly rotating stars are readily produced in binary systems. An accreting star in a binary system can be spun up by mass accretion and quickly approach the break-up limit. Mergers between two stars in a binary are expected to result in massive, fast rotating stars.
C Carathtodory   +7 more
arxiv   +6 more sources

Variable binaries and variables in binaries in the Binary Star Database BDB [PDF]

open access: yesResearch in Astronomy and Astrophysics, 2018
The BDB, Binary star DataBase http://bdb.inasan.ru combines data of the catalogues of binary and multiple stars of all observational types. There is a number of ways for variable stars to form or to be a part of binary or multiple systems. We describe how such stars are represented in the database.
Oleg Malkov   +2 more
arxiv   +5 more sources

The symbiotics as binary stars [PDF]

open access: bronzeInternational Astronomical Union Colloquium, 1982
AbstractSymbiotic stars have become an important testing ground of various theories of binary star evolution. Several physically different models can explain them, but in each case certain fairly restrictive conditions must be met, so if we manage to identify a definite object with a model, it will tell us a lot about the structure and evolutionary ...
M. Plavec
openalex   +3 more sources

Hypervelocity binary stars: smoking gun of massive binary black holes [PDF]

open access: yesAstrophys.J.666:L89-L92,2007, 2007
The hypervelocity stars recently found in the Galactic halo are expelled from the Galactic center through interactions between binary stars and the central massive black hole or between single stars and a hypothetical massive binary black hole. In this paper, we demonstrate that binary stars can be ejected out of the Galactic center with velocities up ...
D. N. C. Lin   +4 more
arxiv   +3 more sources

Star formation environments and the distribution of binary separations [PDF]

open access: yes, 1998
We have carried out K-band speckle observations of a sample of 114 X-ray selected weak-line T Tauri stars in the nearby Scorpius-Centaurus OB association. We find that for binary T Tauri stars closely associated to the early type stars in Upper Scorpius, the youngest subgroup of the OB association, the peak in the distribution of binary separations is ...
Brandner W.   +9 more
arxiv   +4 more sources

Asteroseismology of binary stars and a compilation of core overshoot and rotational frequency values of OB stars [PDF]

open access: yes, 2013
After a brief introduction into the asteroseismic modelling of stars, we provide a compilation of the current seismic estimates of the core overshooting parameter and of the rotational frequency of single and binary massive stars. These important stellar parameters have meanwhile become available for eleven OB-type stars, among which three ...
Aerts, Conny
arxiv   +5 more sources

Pulsed Accretion onto Eccentric and Circular Binaries [PDF]

open access: yes, 2016
We present numerical simulations of circumbinary accretion onto eccentric and circular binaries using the moving-mesh code AREPO. This is the first set of simulations to tackle the problem of binary accretion using a finite-volume scheme on a freely moving mesh, which allows for accurate measurements of accretion onto individual stars for arbitrary ...
Lai, Dong, Muñoz, Diego J.
arxiv   +3 more sources

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