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pro vyhledávání: '"Webbink, Ronald F"'
Autor:
Ge, Hongwei, Tout, Christopher A, Webbink, Ronald F, Chen, Xuefei, Sarkar, Arnab, Li, Jiao, Li, Zhenwei, Zhang, Lifu, Han, Zhanwen
The common envelope evolution (CEE) is vital in forming short orbital period compact binaries. It covers many objects, such as double compact merging binaries, type Ia supernovae progenitors, binary pulsars, and X-ray binaries. Knowledge about the co
Externí odkaz:
http://arxiv.org/abs/2311.17304
The distinguishing feature of the evolution of close binary stars is the role played by the mass exchange between the component stars. Whether the mass transfer is dynamically stable is one of the essential questions in binary evolution. In the limit
Externí odkaz:
http://arxiv.org/abs/2007.09848
Binary evolution is indispensable in stellar evolution to understand the formation and evolution of most peculiar and energetic objects, such as binary compact objects, Type Ia supernovae, X-ray binaries, cataclysmic variables, blue stragglers, hot s
Externí odkaz:
http://arxiv.org/abs/2006.00774
Publikováno v:
Proc. IAU 14 (2018) 449-454
The discovery via gravitational waves of binary black hole systems with total masses greater than $60M_\odot$ has raised interesting questions for stellar evolution theory. Among the most promising formation channels for these systems is one involvin
Externí odkaz:
http://arxiv.org/abs/1811.03656
Adiabatic Mass Loss in Binary Stars. II. From Zero-Age Main Sequence to the Base of the Giant Branch
In the limit of extremely rapid mass transfer, the response of a donor star in an interacting binary becomes asymptotically one of adiabatic expansion. We survey here adiabatic mass loss from Population I stars of mass 0.10 Msun to 100 Msun from the
Externí odkaz:
http://arxiv.org/abs/1507.04843
Akademický článek
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Autor:
Webbink, Ronald F.
The Laser Interferometer Space Antenna (LISA) will open the low-frequency (0.1-100 mHz) part of the gravitational wave spectrum to direct observation. Of order 3600 galactic close binary white dwarfs will be individually resolvable in its all-sky spe
Externí odkaz:
http://arxiv.org/abs/1011.6317
Roche-lobe overflow and common envelope evolution are very important in binary evolution, which is believed to be the main evolutionary channel to hot subdwarf stars. The details of these processes are difficult to model, but adiabatic expansion prov
Externí odkaz:
http://arxiv.org/abs/1005.3105
The asymptotic response of donor stars in interacting binary systems to very rapid mass loss is characterized by adiabatic expansion throughout their interiors. In this limit, energy generation and heat flow through the stellar interior can be neglec
Externí odkaz:
http://arxiv.org/abs/1005.3099
Autor:
Webbink, Ronald F.
Common envelopes form in dynamical time scale mass exchange, when the envelope of a donor star engulfs a much denser companion, and the core of the donor plus the dense companion star spiral inward through this dissipative envelope. As conceived by P
Externí odkaz:
http://arxiv.org/abs/0704.0280