Results 1 to 10 of about 210,765 (341)

Nucleosynthesis of Binary-stripped Stars

The 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, E. Laplace, Jing-ze Ma, S. E. de Mink, S. Justham   +4 more
doaj   +4 more sources

Coalescing Binary Neutron Stars [PDF]

Classical and Quantum Gravity, 1999
Coalescing compact binaries with neutron star or black hole components provide the most promising sources of gravitational radiation for detection by the LIGO/VIRGO/GEO/TAMA laser interferometers now under construction.
Abramovici M, Akmal A, Anderson A, Andersson N, Arras P, Bailes M, Bailyn C D, Baumgarte T W, Baumgarte T W, Baym G, Blanchet L, Carter B, Chandrasekhar S, Choquet-Bruhat Y, Costa E, Curran S J, Danzmann K, Deich W T S, Eichler D, Evans C R, Flanagan E E, Flanagan E E, Frederic A Rasio, Friedman J L, Friedrich H, Goldstein H, Hough J, Iben I Jr, Janka H-T, Junker W, Kidder L E, Kuroda K, Lai D, Lee W H, Lichnerowicz A, Lipunov V M, Lombardi J C, Lombardi J C, Markovic D, Marronetti P, Marronetti P, Matzner R A, Meegan C A, Mészáros P, Mészáros P, Nakamura T, Owen B, Owen B, Paczynski B, Parashar M, Portegies Zwart S F, Rasio F A, Rosswog S, Rosswog S, Rosswog S, Ruffert M, Ruffert M, Ruffert M, Ruffert M, Ruffert M, Schutz B F, Seidel E, Shapiro S L, Shapiro S L, Shibata M, Shibata M, Shibata M, Shibata M, Smarr L, Soberman G E, Stuart L Shapiro, Swesty F D, Symbalisty E M D, Taniguchi K, Tassoul J-L, Thorne K S, Thorne K S, Thorne K S, Thorsett S E, Tutukov A V, van den Heuvel E P J, van Putten M H P M, Wang E Y M, Wang E Y M, Will C M, Wilson J R, Wiseman A G, Wolszczan A   +87 more
core   +5 more sources

The Evolution of Compact Binary Star Systems

Living 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
exaly   +3 more sources

The Evolution of Compact Binary Star Systems

Living Reviews in Relativity, 2006
We review the formation and evolution of compact binary stars consisting of white dwarfs (WDs), neutron stars (NSs), and black holes (BHs). Binary NSs and BHs are thought to be the primary astrophysical sources of gravitational waves (GWs) within the ...
Konstantin A Postnov
exaly   +2 more sources

The symbiotics as binary stars [PDF]

International 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

V1507 CYGNI (HD187399): A Highly Evolved, Enigmatic Interacting Binary System with an Eccentric Orbit

The Astronomical Journal, 2023
The properties of the interacting, eccentric orbit binary V1507 Cyg (HD187399) are examined with spectra that cover wavelengths from 0.63–0.68 μ m. The spectrum of the brightest star is similar to that of the B8 I star β Ori, although with absorption ...
T. J. Davidge
doaj   +1 more source

REVIEW: The Binary Stars

The Astrophysical Journal, 1935
R. G. Aitken
openalex   +4 more sources

NY Bootes: An Active Deep and Low-mass-ratio Contact Binary with a Cool Companion in a Hierarchical Triple System

The Astrophysical Journal, 2023
The first detailed photometric and spectroscopic study of G-type short-period binary NY Boo is presented. The radial velocity curve was obtained by the cross-correlation function (CCF) method based on LAMOST and SDSS spectra, which derived its mass ratio
Fangbin Meng, Liying Zhu, Shengbang Qian, Nianping Liu, Linjia Li, Azizbek Matekov   +5 more
doaj   +1 more source

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

, 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.
Cantiello, Ekström, Izzard, Norbert Langer, Pols, Robert G. Izzard, Selma E. de Mink   +6 more
core   +3 more sources

The binary star

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. Neoclassicism and different movements of “contemporary architecture” run parallel to each other both ...
openaire   +3 more sources