The effects of binary evolution on the dynamics of core collapse and neutron-star kicks
We 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. Interactions with a companion star may change the final rate of rotation, the size of the helium core, the strength of carbon burning...
Main Authors: | Podsiadlowski, P, Langer, N, Poelarends, A, Rappaport, S, Heger, A, Pfahl, E |
---|---|
Format: | Journal article |
Izdano: |
American Astronomical Society
2004
|
Teme: |
Podobne knjige/članki
-
A new class of high-mass X-ray binaries: Implications for core collapse and neutron-star recoil
od: Pfahl, E, et al.
Izdano: (2002) -
Neutron Star Kicks plus Rockets as a Mechanism for Forming Wide Low-eccentricity Neutron Star Binaries
od: Ryosuke Hirai, et al.
Izdano: (2024-01-01) -
A comprehensive study of neutron star retention in globular clusters
od: Pfahl, E, et al.
Izdano: (2002) -
The galactic population of low- and intermediate-Mass X-ray binaries
od: Pfahl, E, et al.
Izdano: (2003) -
Modeling High Mass X-Ray Binaries to Double Neutron Stars through Common Envelope Evolution
od: Yu-Dong Nie, et al.
Izdano: (2025-01-01)