Results 21 to 30 of about 290,820 (278)
Core radii and common-envelope evolution [PDF]
Monthly Notices of the Royal Astronomical Society, 2014 Published in MNRAS. 12 pages, 8 figures.
Hall, Philip D., Tout, Christopher A.
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Black hole formation via hypercritical accretion during common envelope evolution [PDF]
, 1999 Neutron stars inspiralling into a stellar envelope can accrete at rates vastly exceeding the Eddington limit if the flow develops pressures high enough to allow neutrinos to radiate the released gravitational energy.
Abramovici A. +15 more
core +2 more sources
SCATTER: A New Common Envelope Formalism
The Astrophysical Journal, 2023 One of the most mysterious astrophysical states is the common envelope (CE) phase of binary evolution, in which two stars are enshrouded by the envelope shed by one of them. Interactions between the stars and the envelope shrinks the orbit.
Rosanne Di Stefano +4 more
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An alternative to common envelope evolution [PDF]
Monthly Notices of the Royal Astronomical Society, 2007 MNRAS ...
Beer, M. E. +3 more
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Evolution of Neutron-Star, Carbon-Oxygen White-Dwarf Binaries [PDF]
, 2000 At least one, but more likely two or more, eccentric neutron-star, carbon-oxygen white-dwarf binaries with an unrecycled pulsar have been observed.
Braun H. +20 more
core +2 more sources
Common envelope evolution of binary stars [PDF]
Space Science Reviews, 1989 AbstractWe discuss the common envelope phase in the evolution of binary systems. The problem of the efficiency of energy deposition into envelope ejection is treated in some detail. We describe the implications of common envelope evolution for the shaping of planetary nebulae with close binary nuclei and for double white dwarf systems, considered to be
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Progress of Common Envelope Evolution [PDF]
Highlights of Astronomy, 1989 AbstractThe current understanding of the common envelope binary phase of evolution is presented. The results obtained from the detailed computations of the hydrodynamical evolution of this phase demonstrate that the deposition of energy by the double core via frictional processes is sufficiently rapid to drive a mass outflow, primarily in the ...
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The binding energy parameter for common envelope evolution [PDF]
Research in Astronomy and Astrophysics, 2016 The binding energy parameter $ $ plays a vital role in common envelope evolution. Though it is well known that $ $ takes different values for stars with different masses and varies during stellar evolution, it has been erroneously adopted as a constant in most of the population synthesis calculations. We have systematically calculated the values of $
Wang, Cheng, Jia, Kun, Li, Xiang-Dong
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The Astrophysical Journal Letters, 2023 Common envelope (CE) evolution is an outstanding open problem in stellar evolution, critical to the formation of compact binaries including gravitational-wave sources.
M. Renzo +7 more
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Oxygen-neon-rich merger during common envelope evolution [PDF]
Monthly Notices of the Royal Astronomical Society, 2018 We conduct a population synthesis study of the common envelope evolution (CEE) of a white dwarf (WD) and an asymptotic giant branch (AGB) star and find that the potential number of type Ia supernovae (SNe Ia) from the core degenerate (CD) and from the double degenerate (DD) scenarios are of the same order of magnitude.
Canals, Pere +2 more
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