Evolution of the Postmerger Remnants from the Coalescence of Oxygen–Neon and Carbon–Oxygen White Dwarf Pairs

Evolution of the Postmerger Remnants from the Coalescence of Oxygen–Neon and Carbon–Oxygen White Dwarf Pairs

Although multidimensional simulations have investigated the processes of double white dwarf (WD) mergers, postmerger evolution only focused on the carbon–oxygen (CO) or helium (He) WD merger remnants. In this work, we investigate for the first time the evolution of the remnants stemming from the mer...

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Bibliographic Details
Main Authors: Chengyuan Wu, Heran Xiong, Jie Lin, Yunlang Guo, Xiaofeng Wang, Zhanwen Han, Bo Wang
Format: Article
Language:English
Published: IOP Publishing 2023-01-01
Series:The Astrophysical Journal Letters
Subjects:
White dwarf stars
Stellar mergers
Online Access:https://doi.org/10.3847/2041-8213/acb6f3

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