The Path from the Chinese and Japanese Observations of Supernova 1181 AD, to a Type Iax Supernova, to the Merger of CO and ONe White Dwarfs
Bradley E. Schaefer

TL;DR
This paper links the 1181 AD Chinese and Japanese observations of a guest star to the nebula Pa 30, suggesting it resulted from a CO-ONe white dwarf merger leading to a low-luminosity Type Iax supernova, supported by detailed historical and observational evidence.
Contribution
It provides a comprehensive analysis connecting ancient observations to modern supernova remnants, proposing a specific white dwarf merger as the explosion mechanism.
Findings
Historical records constrain the supernova's brightness and duration.
Pa 30's properties match those expected from a white dwarf merger remnant.
No coherent periodic modulations detected in the star's variability.
Abstract
In 1181 AD, Chinese and Japanese observers reported an unmoving bright `Guest Star' in the constellation Chuanshe, visible for 185 days. In 2013, D. Patchick discovered what turned out to be a unique nebula surrounding a unique star, with the structure named `Pa 30', while subsequent workers made connections to mergers of white dwarfs, to the supernova subclass of low-luminosity Type Iax, and to the 1181 transient. Here, I provide a wide range of new observational evidence: First, detailed analysis of the original Chinese and Japanese reports places the `Guest Star' of 1181 into a small region with the only interesting source being Pa 30. Second, the ancient records confidently place the peak magnitude as 0.01.4, and hence peak absolute magnitude 14.516.0 mag. Third, the Pa 30 central star is fading from =14.9 in 1889, to =16.20…
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Taxonomy
TopicsGamma-ray bursts and supernovae
