A possible criterion for envelope ejection in asymptotic giant branch or first giant branch stars
Reads0
Chats0
About:
This article is published in Monthly Notices of the Royal Astronomical Society.The article was published on 1994-09-01 and is currently open access. It has received 318 citations till now. The article focuses on the topics: Asymptotic giant branch & Giant star.read more
Citations
More filters
Journal ArticleDOI
A Comprehensive Study of Binary Compact Objects as Gravitational Wave Sources: Evolutionary Channels, Rates, and Physical Properties
TL;DR: In this article, the authors use population synthesis methods to calculate the properties and coalescence rates of double compact object binaries: double neutron stars, black hole-neutron star systems, and double black holes.
Journal ArticleDOI
Common envelope evolution: where we stand and how we can move forward
Natalia Ivanova,Stephen Justham,Stephen Justham,Xue-Fei Chen,O. De Marco,Chris L. Fryer,Evghenii Gaburov,Hongwei Ge,Evert Glebbeek,Evert Glebbeek,Zhanwen Han,X.-D. Li,G. Lu,G. Lu,T. R. Marsh,Ph. Podsiadlowski,A. Potter,Noam Soker,Ronald E. Taam,Ronald E. Taam,Thomas M. Tauris,Thomas M. Tauris,E.P.J. van den Heuvel,Ronald F. Webbink +23 more
TL;DR: In this paper, the authors present the current best physical understanding of common envelope evolution (CEE) and highlight areas of consensus and disagreement, and stress ideas which should point the way forward for progress in this important but long-standing and largely unconquered problem.
Journal ArticleDOI
The origin of subdwarf B stars – I. The formation channels
TL;DR: In this paper, a detailed investigation of the three main binary evolution channels that can lead to the formation of sdB stars: the common-envelope (CE) ejection channel, the stable Roche lobe overflow (RLOF) channel, and the double helium white dwarfs (WDs) merger channel is presented.
Journal ArticleDOI
The origin of subdwarf B stars – II
TL;DR: In this article, a detailed binary population synthesis (BPS) study of the formation of subdwarf B (sdB) stars and related objects (sdO, sdOB stars) using the latest version of the BPS code developed by Han and co-workers was carried out.
Journal ArticleDOI
The effects of binary evolution on the dynamics of core collapse and neutron star kicks
Ph. Podsiadlowski,Norbert Langer,A. J. T. Poelarends,Saul Rappaport,Alexander Heger,Eric Pfahl +5 more
TL;DR: In this article, the authors systematically examine how the presence in a binary affects the final core structure of a massive star and its consequences for the subsequent supernova explosion, and suggest that the core collapse in an electron-capture supernova (and possibly in the case of relatively small iron cores) leads to a prompt or fast explosion rather than a very slow, delayed neutrino-driven explosion.