The i-process yields of rapidly accreting white dwarfs from multicycle He-shell flash stellar evolution models with mixing parametrizations from 3D hydrodynamics simulations
The i-process yields of rapidly accreting white dwarfs from multicycle He-shell flash stellar evolution models with mixing parametrizations from 3D hydrodynamics simulations
复制标题
DOI：
10.1093/mnras/stz1921
复制
发表时间：
2019-09-01
影响因子：
4.8
通讯作者：
Jones, Samuel
中科院分区：
文献类型：
--
作者：
Denissenkov, Pavel A.;Herwig, Falk;Jones, Samuel
我们模拟了快速吸积CO白色矮星（RAWD）的多周期演化，RAWD具有稳定的11次燃烧，其表面有强烈的He壳层闪光，持续时间为0.7
We have modelled the multicycle evolution of rapidly accreting CO white dwarfs (RAWDs) with stable 11 burning intermittent with strong He-shell flashes on their surfaces for 0.7