The Optically Thick Rotating Magnetic Wind from a Massive White Dwarf Merger Product. II. Axisymmetric Magnetohydrodynamic Simulations

The Optically Thick Rotating Magnetic Wind from a Massive White Dwarf Merger Product. II. Axisymmetric Magnetohydrodynamic Simulations

We numerically construct a series of axisymmetric rotating magnetic wind solutions, aiming at exploring the observation properties of massive white dwarf (WD) merger remnants with a strong magnetic field, a fast spin, and an intense mass loss, as inferred for WD J005311. We investigate the magnetosp...

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Bibliographic Details
Main Authors: Yici Zhong, Kazumi Kashiyama, Shinsuke Takasao, Toshikazu Shigeyama, Kotaro Fujisawa
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal
Subjects:
Stellar winds
White dwarf stars
Stellar rotation
Magnetohydrodynamics
Online Access:https://doi.org/10.3847/1538-4357/ad1f5c

Internet

https://doi.org/10.3847/1538-4357/ad1f5c

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