On the Optical Transients from Double White-dwarf Mergers

On the Optical Transients from Double White-dwarf Mergers

Double white dwarf (DWD) mergers are relevant astrophysical sources expected to produce massive, highly magnetized white dwarfs (WDs), supernovae (SNe) Ia, and neutron stars (NSs). Although they are expected to be numerous sources in the sky, their detection has evaded the most advanced transient su...

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Bibliographic Details
Main Authors: M. F. Sousa, J. G. Coelho, J. C. N. de Araujo, C. Guidorzi, J. A. Rueda
Format: Article
Language:English
Published: IOP Publishing 2023-01-01
Series:The Astrophysical Journal
Subjects:
White dwarf stars
Stellar mergers
Compact binary stars
Compact objects
Visible sources
Online Access:https://doi.org/10.3847/1538-4357/ad022f

Internet

https://doi.org/10.3847/1538-4357/ad022f

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